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Modeling Mg II during Solar Flares. II. Nonequilibrium Effects. To extract the information that the Mg II NUV spectra (observed by the Interface Region Imaging Spectrograph) carry about the chromosphere during solar flares, and to validate models of energy transport via model-data comparison, forward modeling is requir... | [
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Detection of Coronal Mass Ejections at L1 and Forecast of Their Geoeffectiveness. A novel tool aimed to detect solar coronal mass ejections (CMEs) at the Lagrangian point L1 and to forecast their geoeffectiveness is presented in this paper. This approach is based on the analysis of in situ magnetic field and plasma mea... | [
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Measurement of the Nuclear Symmetry Energy Parameters from Gravitational-wave Events. The nuclear symmetry energy plays a role in determining both the nuclear properties of terrestrial matter as well as the astrophysical properties of neutron stars. The first measurement of the neutron star tidal deformability, from gr... | [
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The Relationship of Magnetic Twist and Plasma Motion in a Magnetic Cloud. Our recent investigations indicate that interplanetary magnetic clouds (MCs) have a high-twist core and a weak-twist outer shell. Utilizing the velocity-modified uniform-twist force-free flux rope model, we further investigate the relationship be... | [
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Isotopes of Barium as a Chronometer for Supernova Dust Formation. Ejecta from the explosion of massive stars (core-collapse supernovae) make an important contribution to dust in the interstellar medium. However, dust formation around supernovae is not a simple process, with the formation of several components over time... | [
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A Supernova Remnant Counterpart for HESS J1832-085. We examine the new Galactic supernova remnant (SNR) candidate, G23.11+0.18, as seen by the Murchison Widefield Array radio telescope. We describe the morphology of the candidate and find a spectral index of -0.63 ± 0.05 in the 70-170 MHz domain. Coincident TeV gamma-r... | [
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Trigonometric Parallaxes of High-mass Star-forming Regions: Our View of the Milky Way. We compile and analyze approximately 200 trigonometric parallaxes and proper motions of molecular masers associated with very young high-mass stars. Most of the measurements come from the BeSSeL Survey using the VLBA and the Japanese... | [
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Can the Uranian Satellites Form from a Debris Disk Generated by a Giant Impact?. Hydrodynamic simulations of a giant impact to proto-Uranus indicated that such an impact could tilt its rotational axis and produce a circumplanetary debris disk beyond the corotation radius of Uranus. However, whether Uranian satellites c... | [
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Sensitivity of Super-Kamiokande with Gadolinium to Low Energy Antineutrinos from Pre-supernova Emission. Supernova detection is a major objective of the Super-Kamiokande (SK) experiment. In the next stage of SK (SK-Gd), gadolinium (Gd) sulfate will be added to the detector, which will improve the ability of the detecto... | [
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Measurements of Low Temperature Rate Coefficients for the Reaction of CH with CH<SUB>2</SUB>O and Application to Dark Cloud and AGB Stellar Wind Models. Rate coefficients have been measured for the reaction of CH radicals with formaldehyde, CH2O, over the temperature range of 31-133 K using a pulsed Laval nozzle appara... | [
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Nuclear Ignition of White Dwarf Stars by Relativistic Encounters with Rotating Intermediate Mass Black Holes. We present results from general relativistic calculations of nuclear ignition in white dwarf stars triggered by near encounters with rotating intermediate mass black holes with different spin and alignment para... | [
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Steady Electron Runaway Model SERM: Astrophysical Alternative for the Maxwellian Assumption. A Steady Electron Runaway Model (SERM) is formulated describing plasmas in the astrophysical “condition” having finite (rather than infinitesimal) Knudsen number, {K}}}Pe}, suggesting an omnipresent leptokurtic, nonthermal, and... | [
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Fluorine Abundances in the Galactic Disk. The chemical evolution of fluorine is investigated in a sample of Milky Way red giant stars that span a significant range in metallicity from [Fe/H] ∼ -1.3 to 0.0 dex. Fluorine abundances are derived from vibration-rotation lines of HF in high-resolution infrared spectra near 2... | [
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On the Source Position and Duration of a Solar Type III Radio Burst Observed by LOFAR. The flux of solar type III radio bursts have a time profile of rising and decay phases at a given frequency, which has been actively studied since the 1970s. Several factors that may influence the duration of a type III radio burst h... | [
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NuSTAR and Chandra Observations of New X-Ray Transients in the Central Parsec of the Galaxy. We report NuSTAR and Chandra observations of two X-ray transients, SWIFT J174540.7-290015 (T15) and SWIFT J174540.2-290037 (T37), which were discovered by the Neil Gehrels Swift Observatory in 2016 within r ∼ 1 pc of Sgr A*. Nu... | [
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Testing Stellar Evolution with Asteroseismic Inversions of a Main-sequence Star Harboring a Small Convective Core. The goal of stellar evolution theory is to predict the structure of stars throughout their lifetimes. Usually, these predictions can be assessed only indirectly, for example by comparing predicted and obse... | [
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Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?. Rapid rotation is a fundamental characteristic of classical Be stars and a crucial property allowing for the formation of their circumstellar disks. Past evolution in a mass and angular momentum transferring binary system offers a pl... | [
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The Long-standing Closure Crisis in Coronal Plasmas. Coronal and solar wind physics have long used plasma fluid models to motivate physical explanations of observations; the hypothesized model is introduced into a fluid simulation to see if observations are reproduced. This procedure is called Verification of Mechanism... | [
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Measurement of the Extragalactic Background Light Spectral Energy Distribution with VERITAS. The extragalactic background light (EBL), a diffuse photon field in the optical and infrared range, is a record of radiative processes over the universe’s history. Spectral measurements of blazars at very high energies (>100... | [
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Population Synthesis of Black Hole Binaries with Normal-star Companions. I. Detached Systems. Optical observations of normal stars in binary systems with massive unseen objects have been proposed to search for candidate black holes (BHs) and provide a direct measurement of their dynamical masses. In this paper, we have... | [
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Orbital Evolution of Eccentric Low-mass Companions Embedded in Gaseous Disks: Testing the Local Approximation. We study the tidal interaction between a low-mass companion (e.g., a protoplanet or a black hole) in orbit about a central mass, and the accretion disk within which it is submerged. We present results for a co... | [
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The M101 Satellite Luminosity Function and the Halo-Halo Scatter among Local Volume Hosts. We have obtained deep Hubble Space Telescope (HST) imaging of 19 dwarf galaxy candidates in the vicinity of M101. Advanced Camera for Surveys HST photometry for two of these objects showed resolved stellar populations and tip of ... | [
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Spectral Diagnostics of Cool Flare Loops Observed by the SST. I. Inversion of the Ca II 8542 Å and Hβ Lines. Flare loops form an integral part of eruptive events, being detected in the range of temperatures from X-rays down to cool chromospheric-like plasmas. While hot loops are routinely observed by the Solar Dynamics... | [
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Chromospheric UV Bursts and Turbulent-driven Magnetic Reconnection. We use Interface Region Imaging Spectrograph (IRIS) spacecraft data to study a group of Chromospheric ultraviolet bursts (UVBs) associated with an active region. We classify the UVBs into two types: smaller ones that can only be measured once by the sc... | [
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Exploring the Asymmetry of the Solar Corona Electron Density with Very Long Baseline Interferometry. The Sun’s corona has interested researchers for multiple reasons, including the search for a solution to the famous coronal heating problem and a purely practical consideration of predicting geomagnetic storms on Earth.... | [
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A Cepheid-based Distance to the Seyfert Galaxy NGC 6814. We present a Cepheid-based distance to the nearby Seyfert galaxy NGC 6814 from Hubble Space Telescope observations. We obtained F555W and F814W imaging over the course of 12 visits with logarithmic time spacing in 2013 August-October. We detected and made photome... | [
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VER J2227+608: A Hadronic PeVatron Pulsar Wind Nebula?. We report the detection of GeV γ-ray emission from the very-high-energy γ-ray source VER J2227+608 associated with the “tail” region of supernova remnant (SNR) G106.3+2.7. The GeV γ-ray emission is extended and spatially coincident with molecular clouds traced by ... | [
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Oscillator Strengths for the Lyman and Werner Bands of Molecular Hydrogen Studied by the Dipole (γ, γ) Method. Absolute optical oscillator strength (OOS) plays an extremely important role in molecular astrophysics research, especially for hydrogen. In this work, a novel dipole (γ, γ) method is used to determine the abs... | [
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Coronae of Zero/Low-metal, Low-mass Stars. Recent theoretical studies suggest the existence of low-mass, zero-metal stars in the current universe. To study the basic properties of the atmosphere of low-mass first stars, we perform one-dimensional magnetohydrodynamical simulations for the heating of coronal loops on low... | [
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Investigating Early-type Galaxy Evolution with a Multiwavelength Approach. III. Insights from SPH Simulations with Chemophotometric Implementation. We are exploring galaxy evolution in low-density environments exploiting smooth particle hydrodynamic simulations, including chemophotometric implementation. From a large g... | [
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Diagnostics of Collisions between Electrons and Water Molecules in Near-ultraviolet and Visible Wavelengths. We studied the dissociation reactions of electron impact on water vapor for several fragment species at optical and near-ultraviolet wavelengths (200-850 nm). The resulting spectrum is dominated by the hydrogen ... | [
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A NICER Thermonuclear Burst from the Millisecond X-Ray Pulsar SAX J1808.4-3658. The Neutron Star Interior Composition Explorer (NICER) has extensively monitored the 2019 August outburst of the 401 Hz millisecond X-ray pulsar SAX J1808.4-3658. In this Letter, we report on the detection of a bright helium-fueled Type I X... | [
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Inferring the Presence of Tides in Detached White Dwarf Binaries. Tidal interactions can play an important role as compact white dwarf (WD) binaries are driven together by gravitational waves (GWs). This will modify the strain evolution measured by future space-based GW detectors and impact the potential outcome of the... | [
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HSC-XD 52: An X-Ray Detected AGN in a Low-mass Galaxy at z ∼ 0.56. The properties of low-mass galaxies hosting central black holes provide clues about the formation and evolution of the progenitors of supermassive black holes. In this Letter, we present HSC-XD 52, a spectroscopically confirmed low-mass active galactic ... | [
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Varstrometry for Off-nucleus and Dual Sub-Kpc AGN (VODKA): How Well Centered Are Low-z AGN?. Off-nucleus active galactic nuclei (AGN) can be signposts of inspiraling supermassive black holes (SMBHs) on galactic scales, or accreting SMBHs recoiling after the coalescence of an SMBH binary or slingshot from three-body int... | [
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Ion Cyclotron Waves in Field-aligned Solar Wind Turbulence. The nature of the solar wind parallel fluctuations is investigated in this Letter by using magnetic helicity to characterize their polarization state at proton scales. Our aim is to assess the role of the proton cyclotron instability as a mechanism for generat... | [
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The Influence of Gas-phase Chemistry on Organic Haze Formation. Although photochemically produced organic hazes are common in planetary atmospheres, there have been few experimental investigations of the gas-phase chemistry leading to organic haze formation. We report a laboratory study of the gas-phase compounds forme... | [
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The First Detection of a Low-frequency Turnover in Nonthermal Emission from the Jet of a Young Star. Radio emission in jets from young stellar objects (YSOs) in the form of nonthermal emission has been seen toward several YSOs. Thought to be synchrotron emission from strong shocks in the jet, it could provide valuable ... | [
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Comparing the Quenching Times of Faint M31 and Milky Way Satellite Galaxies. We present the star formation histories (SFHs) of 20 faint M31 satellites (-12 ≲ M V ≲ -6) that were measured by modeling sub-horizontal branch depth color-magnitude diagrams constructed from Hubble Space Telescope (HST) imaging. Reinforcing... | [
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Detection of CN Gas in Interstellar Object 2I/Borisov. The detection of interstellar objects passing through the solar system offers the promise of constraining the physical and chemical processes involved in planetary formation in other extrasolar systems. While the effect of outgassing by 1I/2017 U1 (’Oumuamua) was d... | [
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Detection of Pulses from the Vela Pulsar at Millimeter Wavelengths with Phased ALMA. We report on the first detection of pulsed radio emission from a radio pulsar with the Atacama Large Millimeter/submillimeter Array (ALMA) telescope. The detection was made in the Band-3 frequency range (85-101 GHz) using ALMA in the p... | [
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Round-trip Slipping Motion of the Circular Flare Ribbon Evidenced in a Fan-spine Jet. A solar jet that occurred on 2014 July 31, which was accompanied by a GOES C1.3 flare and a mini-filament eruption at the jet base, was studied by using observations taken by the New Vacuum Solar Telescope and the Solar Dynamic Observ... | [
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Four Newborn Planets Transiting the Young Solar Analog V1298 Tau. Exoplanets orbiting pre-main-sequence stars are laboratories for studying planet evolution processes, including atmospheric loss, orbital migration, and radiative cooling. V1298 Tau, a young solar analog with an age of 23 ± 4 Myr, is one such laboratory.... | [
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The Evolution of Baryonic Mass Function of Galaxies to z = 3. We combine the published stellar mass function (SMF) and gas scaling relations to explore the baryonic (stellar plus cold gas) mass function (BMF) of galaxies to redshift z = 3. We find evidence that at log(M baryon/M ⊙) > 11.3, the BMF has evolved little... | [
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First Detection of Plasmoids from Breakout Reconnection on the Sun. Transient collimated plasma ejections (jets) occur frequently throughout the solar corona, in active regions, quiet Sun, and coronal holes. Although magnetic reconnection is generally agreed to be the mechanism of energy release in jets, the factors th... | [
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Auroral Beads at Saturn and the Driving Mechanism: Cassini Proximal Orbits. During the Grand Finale Phase of Cassini, the Ultraviolet Imaging Spectrograph on board the spacecraft detected repeated detached small-scale auroral structures. We describe these structures as auroral beads, a term introduced in the terrestria... | [
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Lorentz Force Evolution Reveals the Energy Build-up Processes during Recurrent Eruptive Solar Flares. The energy release and build-up processes in the solar corona have significant implications in particular for the case of large recurrent flares, which pose challenging questions about the conditions that lead to the e... | [
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Collapse of the General Circulation in Shortwave-absorbing Atmospheres: An Idealized Model Study. The response of the general circulation in a dry atmosphere to various atmospheric shortwave absorptivities is investigated in a three-dimensional general circulation model with gray radiation. Shortwave absorption in the ... | [
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GROWTH on S190425z: Searching Thousands of Square Degrees to Identify an Optical or Infrared Counterpart to a Binary Neutron Star Merger with the Zwicky Transient Facility and Palomar Gattini-IR. The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the... | [
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The Nuclear Filaments inside the Circumnuclear Disk in the Central 0.5 pc of the Galactic Center. We present CS(7-6) line maps toward the central parsec of the Galactic center, conducted with the Atacama Large Millimeter/submillimeter Array. The primary goal is to find and characterize the gas structure in the inner ca... | [
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How to Fuel an AGN: Mapping Circumnuclear Gas in NGC 6240 with ALMA. Dynamical black hole mass measurements in some gas-rich galaxy mergers indicate that they are overmassive relative to their host galaxy properties. Overmassive black holes in these systems present a conflict with the standard progression of galaxy mer... | [
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Half-mass Radii of Quiescent and Star-forming Galaxies Evolve Slowly from 0 ≲ z ≤ 2.5: Implications for Galaxy Assembly Histories. We use high-resolution, multiband imaging of ∼16,500 galaxies in the CANDELS fields at 0 ≲ z ≤ 2.5 to study the evolution of color gradients and half-mass radii over cosmic time. We find th... | [
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SN2018kzr: A Rapidly Declining Transient from the Destruction of a White Dwarf. We present SN2018kzr, the fastest declining supernova-like transient, second only to the kilonova, AT2017gfo. SN2018kzr is characterized by a peak magnitude of M r = -17.98, a peak bolometric luminosity of ∼1.4 × 1043 erg s-1, and a rapid... | [
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The Precision of Mass Measurements Required for Robust Atmospheric Characterization of Transiting Exoplanets. Two of Transiting Exoplanet Survey Satellite’s major science goals are to measure masses for 50 planets smaller than 4 Earth radii and to discover high-quality targets for atmospheric characterization efforts. ... | [
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Propagation of Solar Energetic Particles in the Outer Heliosphere: Interplay between Scattering and Adiabatic Focusing. The turbulence and spatial nonuniformity of the guide magnetic field cause two competitive effects, namely, the scattering effect and the adiabatic focusing effect, respectively. In this work, we nume... | [
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Constraining Planetary Gas Accretion Rate from Hα Line Width and Intensity: Case of PDS 70 b and c. Recent observations of protoplanets embedded in circumstellar disks have shed light on the planet formation process. In particular, detection of hydrogen Balmer-line (Hα) emission gives direct constraints on late-stage a... | [
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Direct Detection of Solar Angular Momentum Loss with the Wind Spacecraft. The rate at which the solar wind extracts angular momentum (AM) from the Sun has been predicted by theoretical models for many decades, and yet we lack a conclusive measurement from in situ observations. In this Letter we present a new estimate o... | [
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Mapping Electron Temperature Variations across a Spiral Arm in NGC 1672. We report one of the first extragalactic observations of electron temperature variations across a spiral arm. Using Multi Unit Spectroscopic Explorer mosaic observations of the nearby galaxy NGC 1672, we measure the [N II]λ5755 auroral line in a s... | [
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Molecular Gas in the Outflow of the Small Magellanic Cloud. We report the first evidence of molecular gas in two atomic hydrogen (H I) clouds associated with gas outflowing from the Small Magellanic Cloud (SMC). We used the Atacama Pathfinder Experiment to detect and spatially resolve individual clumps of 12CO(2 → 1) e... | [
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The Shadow of a Spherically Accreting Black Hole. We explore a simple spherical model of optically thin accretion on a Schwarzschild black hole, and study the properties of the image as seen by a distant observer. We show that a dark circular region in the center—a shadow—is always present. The outer edge of the shadow... | [
"http://astrothesaurus.org/uat/14",
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Stellar Velocity Dispersion of a Massive Quenching Galaxy at z = 4.01. We present the first stellar velocity dispersion measurement of a massive quenching galaxy at z = 4. The galaxy is first identified as a massive z ≥ 4 galaxy with suppressed star formation from photometric redshifts based on deep multiband data. A f... | [
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Dark Matter Signatures of Supermassive Black Hole Binaries. A natural consequence of the galaxy formation paradigm is the existence of supermassive black hole (SMBH) binaries. Gravitational perturbations from a far-away SMBH companion can induce high orbital eccentricities on dark matter (DM) particles orbiting the pri... | [
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The Galaxy’s Gas Content Regulated by the Dark Matter Halo Mass Results in a Superlinear M <SUB>BH</SUB>-M <SUB>⋆</SUB> Relation. Supermassive black holes (SMBHs) are tightly correlated with their hosts, but the origin of such connection remains elusive. To explore the cosmic buildup of this scaling relation, we presen... | [
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Wide Bandwidth Observations of Pulsars C, D, and J in 47 Tucanae. We report the first wide-band observations of pulsars C, D, and J in the globular cluster 47 Tucanae (NGC 104) using the Ultra-Wideband Low (UWL) receiver system recently installed on the Parkes 64 m radio telescope. The wide frequency range of the UWL r... | [
"http://astrothesaurus.org/uat/656",
"http://astrothesaurus.org/uat/1306",
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Constraining X-Ray Coronal Size with Transverse Motion of AGN Ultra-fast Outflows. One of the canonical physical properties of ultra-fast outflows (UFOs) seen in a diverse population of active galactic nuclei is its seemingly very broad width (i.e., ∆v ≳ 10,000 km s-1), a feature often required for X-ray spectral model... | [
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"http://astrothesaurus.org/uat/1447",
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"http://astrothesaurus.org/uat/672",
"http://astrothesaurus.org/uat/1319",
"http://astrothesaurus.org/uat/1435",
"http://astrothesaurus.org/uat/1545"
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First Detection of Submillimeter-wave [<SUP>13</SUP>C I] <SUP>3</SUP> P <SUB>1</SUB>-<SUP>3</SUP> P <SUB>0</SUB> Emission in a Gaseous Debris Disk of 49 Ceti with ALMA. We have detected the submillimeter-wave fine-structure transition (3 P 1-3 P 0) of 13C, [13C I], in the gaseous debris disk of 49 Ceti with the Atacama... | [
"http://astrothesaurus.org/uat/1145",
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"Observational astronomy",
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Organosulfur Compounds Formed by Sulfur Ion Bombardment of Astrophysical Ice Analogs: Implications for Moons, Comets, and Kuiper Belt Objects. Carbon, hydrogen, nitrogen, oxygen, and sulfur are the main elements involved in the solid-phase chemistry of various astrophysical environments. Among these elements, sulfur ch... | [
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"http://astrothesaurus.org/uat/74",
"http://astrothesaurus.org/uat/1705",
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The Interstellar Object ’Oumuamua as a Fractal Dust Aggregate. The first known interstellar object ’Oumuamua exhibited a nongravitational acceleration that appeared inconsistent with cometary outgassing, leaving radiation pressure as the most likely force. Barring the alien lightsail hypothesis, an ultra-low density du... | [
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Determination of Transport Coefficients by Coronal Seismology of Flare-induced Slow-mode Waves: Numerical Parametric Study of a 1D Loop Model. Recent studies of a flaring loop oscillation event on 2013 December 28 observed by the Atmospheric Imaging Assembly of the Solar Dynamics Observatory have revealed the suppressi... | [
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Rankine-Hugoniot Shock Conditions for Space and Astrophysical Plasmas Described by Kappa Distributions. This paper provides the set of Rankine-Hugoniot (R-H) jump conditions for shocks in space and astrophysical plasmas described by kappa, distributions. The characteristic result is the development of a new R-H conditi... | [
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Can Neutron-star Mergers Explain the r-process Enrichment in Globular Clusters?. Star-to-star dispersion of r-process elements has been observed in a significant number of old, metal-poor globular clusters (GCs). We investigate early-time neutron-star mergers as the mechanism for this enrichment. Through both numerical... | [
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The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. I. Identifying and Characterizing the Protostellar Content of the OMC-2 FIR4 and OMC-2 FIR3 Regions. We present Atacama Large Millimeter/submillimeter Array (0.87 mm) and Very Large Array (9 mm) observations toward OMC-2 FIR4 and OMC-2 FIR3... | [
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Dwarfs or Giants? Stellar Metallicities and Distances from ugrizG Multiband Photometry. We present a new fully data-driven algorithm that uses photometric data from the Canada-France Imaging Survey (CFIS; u), Pan-STARRS 1 (PS1; griz), and Gaia (G) to discriminate between dwarf and giant stars and to estimate their dist... | [
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Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events. Low-background searches for astrophysical neutrino sources anywhere in the sky can be performed using cascade events induced by neutrinos of all flavors interacting in IceCube with energies as low as ∼1 TeV. Previously we showed ... | [
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UVIT Open Cluster Study. II. Detection of Extremely Low Mass White Dwarfs and Post-Mass Transfer Binaries in M67. A detailed study of the UV-bright stars in the old open star cluster M67 is presented based on the far-UV observations using the Ultra Violet Imaging Telescope (UVIT) on ASTROSAT. The UV and UV-optical colo... | [
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Habitability and Spectroscopic Observability of Warm M-dwarf Exoplanets Evaluated with a 3D Chemistry-Climate Model. Planets residing in circumstellar habitable zones offer us the best opportunities to test hypotheses of life’s potential pervasiveness and complexity. Constraining the precise boundaries of habitability ... | [
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Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies. Magnetic fields are ubiquitous in the interstellar medium but notoriously difficult to study through observation. Making use of the advances in our understanding of MHD turbulence and turbulent reconnection, the velocity gradients ... | [
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Sunspot Characteristics at the Onset of the Maunder Minimum Based on the Observations of Hevelius. An analysis of the sunspot observations made by Hevelius during 1642-1645 is presented. These records are the only systematic sunspot observations just before the Maunder Minimum (MM). We have studied different phenomena ... | [
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Lyα Observations of High Radial Velocity Low-mass Stars Ross 1044 and Ross 825. The discovery of habitable zone (HZ) planets around low-mass stars has highlighted the need for a comprehensive understanding of the radiation environments in which such planets reside. Of particular importance is knowledge of the far-ultra... | [
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Evolution of ONeMg Core in Super-AGB Stars toward Electron-capture Supernovae: Effects of Updated Electron-capture Rate. Stars with ∼8-10 M ⊙ evolve to form a strongly degenerate ONeMg core. When the core mass becomes close to the Chandrasekhar mass, the core undergoes electron captures on 24Mg and 20Ne that induce an ... | [
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A Two-zone Model for Blazar Emission: Implications for TXS 0506+056 and the Neutrino Event IceCube-170922A. A high-energy muon neutrino event, IceCube-170922A, was recently discovered in both spatial and temporal coincidence with a gamma-ray flare of the blazar TXS 0506+056. It has been shown with standard one-zone mod... | [
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A Search for Late-time Radio Emission and Fast Radio Bursts from Superluminous Supernovae. We present results of a search for late-time radio emission and fast radio bursts (FRBs) from a sample of type-I superluminous supernovae (SLSNe-I). We used the Karl G. Jansky Very Large Array to observe 10 SLSN-I more than 5 yr ... | [
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The Atmospheric Circulation of Ultra-hot Jupiters. Recent observations of ultra-hot Jupiters with dayside temperatures in excess of 2500 K have found evidence for new physical processes at play in their atmospheres. In this work, we investigate the effects of the dissociation of molecular hydrogen and recombination of ... | [
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Type IIP Supernova Progenitors and Their Explodability. I. Convective Overshoot, Blue Loops, and Surface Composition. We present the evolution of massive star progenitors of supernovae of type IIP. We take the example of the nearby and well-studied SN 2013ej. We explore how convective overshoot affects the stellar stru... | [
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Understanding the Discrepancy between IRX and Balmer Decrement in Tracing Galaxy Dust Attenuation. We compare the infrared excess (IRX) and Balmer decrement ({{H}}α /{{H}}β ) as dust attenuation indicators in relation to other galaxy parameters using a sample of ∼32,000 local star-forming galaxies (SFGs) carefully sele... | [
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Fast Outflows Identified in Early Star-forming Galaxies at z = 5-6. We present velocities of galactic outflows in seven star-forming galaxies at z = 5-6 with stellar masses of M * ∼ 1010.1 {M}⊙ . Although it is challenging to observationally determine the outflow velocities, we overcome this by using ALMA [C II] 158 μm... | [
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A Carbon-rich Hot Bubble in the Planetary Nebula NGC 5189. We present the discovery of extended X-ray emission from the planetary nebula (PN) NGC 5189 around the [WO1]-type WD 1330-657 with XMM-Newton. The X-ray-emitting gas fills the cavities detected in the Hubble Space Telescope [O III] narrowband image and presents... | [
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The Mass-Metallicity Relation at z ∼ 0.8: Redshift Evolution and Parameter Dependency. The spectra of emission-line galaxies from the extended Baryon Oscillation Spectroscopic Survey of the Sloan Digit Sky Survey (SDSS) are used to study the mass-metallicity relation (MZR) at z ∼ 0.8. The selected sample contains about... | [
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Frequency Distribution of Acoustic Oscillation in the Solar Atmosphere During Flare Event. We present a study of multi-wavelength observations, of a C 2.3 solar flare in Active Region NOAA 12353, observed on 2015 May 23, which reveal new properties of acoustic waves in the flaring region. The space-, and ground-based d... | [
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Mid-IR Variability and Dust Reverberation Mapping of Low-z Quasars. I. Data, Methods, and Basic Results. The continued operation of the Wide-field Infrared Survey Explorer (WISE), combined with several ground-based optical transient surveys (e.g., CRTS, ASAS-SN, and PTF), offers an unprecedented opportunity to explore ... | [
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Age Determination of Galactic B-type Stars in Double-lined Eclipsing Binaries. We present the results of age determination for galactic B-type main-sequence stars that are components of double-lined eclipsing binaries. Only detached systems are considered. We analyze 38 binary systems that meet such criteria. The analy... | [
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The Interface between the Outer Heliosphere and the Inner Local ISM: Morphology of the Local Interstellar Cloud, Its Hydrogen Hole, Strömgren Shells, and <SUP>60</SUP>Fe Accretion. We describe the interface between the outer heliosphere and the local interstellar medium (LISM) surrounding the Sun. The components of the... | [
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"http://astrothesaurus.org/uat/1642",
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The Radius-Luminosity Relationship Depends on Optical Spectra in Active Galactic Nuclei. The radius-luminosity ({R}{{H}β }{--}{L}5100) relationship of active galactic nuclei (AGNs) established by the reverberation mapping (RM) observations has been widely used as a single-epoch black hole mass estimator in the research... | [
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On Doppler Shift and Its Center-to-limb Variation in Active Regions in the Transition Region. A comprehensive understanding of the structure of Doppler motions in the transition region including the center-to-limb variation and its relationship with the magnetic field structure is vital for the understanding of mass an... | [
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"http://astrothesaurus.org/uat/1693",
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"http://astrothesaurus.org/uat/1503",
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Nucleosynthesis Constraints on the Energy Growth Timescale of a Core-collapse Supernova Explosion. Details of the explosion mechanism of core-collapse supernovae (CCSNe) are not yet fully understood. There are an increasing number of numerical examples by ab initio core-collapse simulations leading to an explosion. Mos... | [
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"http://astrothesaurus.org/uat/1664",
"http://astrothesaurus.org/uat/1131",
"http://astrothesaurus.org/uat/304",
"http://astrothesaurus.org/uat/1668"
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Mining for Dark Matter Substructure: Inferring Subhalo Population Properties from Strong Lenses with Machine Learning. The subtle and unique imprint of dark matter substructure on extended arcs in strong-lensing systems contains a wealth of information about the properties and distribution of dark matter on small scale... | [
"http://astrothesaurus.org/uat/343",
"http://astrothesaurus.org/uat/1903",
"http://astrothesaurus.org/uat/1886",
"http://astrothesaurus.org/uat/1938",
"http://astrothesaurus.org/uat/1643",
"http://astrothesaurus.org/uat/670",
"http://astrothesaurus.org/uat/353"
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"Nonparametric inference",
"Astrostatistics techniques",
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"http://astrothesaurus.org/uat/1684",
"http://astrothesaurus.org/uat/1933",
"http://astrothesaurus.org/uat/2088",
"http://astrothesaurus.org/uat/2256",
"http://astrothesaurus.org/uat/2347"
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High Angular Resolution ALMA Images of Dust and Molecules in the SN 1987A Ejecta. We present high angular resolution (∼80 mas) ALMA continuum images of the SN 1987A system, together with CO J = 2 \to 1, J = 6 \to 5, and SiO J = 5 \to 4 to J = 7 \to 6 images, which clearly resolve the ejecta (dust continuum and molecule... | [
"http://astrothesaurus.org/uat/836",
"http://astrothesaurus.org/uat/849",
"http://astrothesaurus.org/uat/1668"
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"http://astrothesaurus.org/uat/1779",
"http://astrothesaurus.org/uat/2129",
"http://astrothesaurus.org/uat/2167"
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