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Evidence of Nonluminous Matter in the Center of M62. Theoretical models suggest that intermediate-mass black holes (IMBHs) may form and reside in the centers of globular clusters. IMBHs are still elusive to observations, but the accelerations of pulsars may bring along a unique fingerprint of their presence. In this wo... | [
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Torus Constraints in ANEPD-CXO245: A Compton-thick AGN with Double-peaked Narrow Lines. We report on the torus constraints of the Compton-thick active galactic nucleus (AGN) with double-peaked optical narrow-line region emission lines, ANEPD-CXO245, at z = 0.449 in the AKARI NEP Deep Field. The unique infrared data on ... | [
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A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass. Super spirals are the most massive star-forming disk galaxies in the universe. We measured rotation curves for 23 massive spirals with the Southern African Large Telescope (SALT) and found a wide range of fast rotation speeds (240-570 km s-1)... | [
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Where Are the Electromagnetic-wave Counterparts of Stellar-mass Binary Black Hole Mergers?. Multimessenger astronomy, combining gravitational-wave (GW) and electromagnetic-wave (EM) observations, has a huge impact on physics, astrophysics, and cosmology. However, the majority of sources detected with currently running ... | [
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Coronal Response to Magnetically Suppressed CME Events in M-dwarf Stars. We report the results of the first state-of-the-art numerical simulations of coronal mass ejections (CMEs) taking place in realistic magnetic field configurations of moderately active M-dwarf stars. Our analysis indicates that a clear, novel, and ... | [
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Long-standing Small-scale Reconnection Processes at Saturn Revealed by Cassini. The internal mass source from the icy moon Enceladus in Saturn’s rapidly rotating magnetosphere drives electromagnetic dynamics in multiple spatial and temporal scales. The distribution and circulation of the internal plasma and associated ... | [
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New Candidate Planetary Nebulae in Galactic Globular Clusters from the VVV Survey. Only four globular cluster planetary nebulae (GCPN) are known so far in the Milky Way. About 50 new globular clusters have been recently discovered toward the Galactic bulge. We present a search for planetary nebulae within 3′ of the new... | [
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Searching for Hypermassive Neutron Stars with Short Gamma-Ray Bursts. Neutron star mergers can form a hypermassive neutron star (HMNS) remnant, which may be the engine of a short gamma-ray burst (SGRB) before it collapses to a black hole, possibly several hundred milliseconds after the merger. During the lifetime of an... | [
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Multi-TeV Flaring from High-energy Blazars: An Evidence of the Photohadronic Process. High-energy peaked blazars are known to undergo episodes of flaring in GeV-TeV gamma-rays involving different timescales. This flaring mechanism is not well understood, despite long-term simultaneous multiwavelength observations. Thes... | [
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The Earliest Candidates of Auroral Observations in Assyrian Astrological Reports: Insights on Solar Activity around 660 BCE. Auroral records found in historical archives and cosmogenic isotopes found in natural archives have served as sound proxies of coronal mass ejections and solar energetic particles (SEPs), respect... | [
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Evidence for Low Radiative Efficiency or Highly Obscured Growth of z > 7 Quasars. The supermassive black holes (SMBHs) observed at the centers of all massive galaxies are believed to have grown via luminous accretion during quasar phases in the distant past. The fraction of inflowing rest mass energy emitted as ligh... | [
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COS Observations of the Cosmic Web: A Search for the Cooler Components of a Hot, X-Ray Identified Filament. In the local universe, a large fraction of the baryon content is believed to exist as diffuse gas in filaments. While this gas is directly observable in X-ray emission around clusters of galaxies, it is primarily... | [
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X-Ray Fluorescence from Super-Eddington Accreting Black Holes. X-ray reverberation has proven to be a powerful tool capable of probing the innermost region of accretion disks around compact objects. Current theoretical effort generally assumes that the disk is geometrically thin, optically thick, and orbiting with Kepl... | [
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Hidden Planets: Implications from ’Oumuamua and DSHARP. The discovery of ’Oumuamua (1I/2017 U1), the first interstellar interloper, suggests an abundance of free-floating small bodies whose ejection into galactic space cannot be explained by the current population of confirmed exoplanets. Shortly after ’Oumuamua’s disc... | [
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A Family Picture: Tracing the Dynamical Path of the Structural Properties of Multiple Populations in Globular Clusters. We studied the spatial distributions of multiple stellar populations (MPs) in a sample of 20 globular clusters (GCs) spanning a broad range of dynamical ages. The differences between first-population ... | [
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The Star Formation History and Dynamics of the Ultra-diffuse Galaxy Dragonfly 44 in MOND and MOG. The observed line-of-sight velocity dispersion σ los of the ultra-diffuse galaxy Dragonfly 44 (DF44) requires a Newtonian dynamical mass-to-light ratio of {M}dyn}/{L}I={26}-6+7 solar units. This is well outside the accepta... | [
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The FRB 121102 Host Is Atypical among Nearby Fast Radio Bursts. We search for host galaxy candidates of nearby fast radio bursts (FRBs), FRB 180729.J1316+55, FRB 171020, FRB 171213, FRB 180810.J1159+83, and FRB 180814.J0422+73 (the second repeating FRB). We compare the absolute magnitudes and the expected host dispersi... | [
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Molecular Cloud Origin for Oxygen Isotopic Heterogeneity Recorded by a Primordial Spinel-rich Refractory Inclusion. A spinel-rich, layered calcium- aluminum-rich spherule from the MIL 090019 CO3 chondrite contains a spinel core with a relatively 16O-rich (Δ17O ∼ -18‰) and mass-fractionated oxygen isotopic composition s... | [
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The Physical Origins of the Identified and Still Missing Components of the Warm-Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113. The relationship between galaxies and the state/chemical enrichment of the warm-hot intergalactic medium (WHIM) expected to dominate the baryon budget ... | [
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The Reliability of the Low-latency Estimation of Binary Neutron Star Chirp Mass. The LIGO and Virgo Collaborations currently conduct searches for gravitational waves from compact binary coalescences in real time. For promising candidate events, a sky map and distance estimation are released in low latency to facilitate... | [
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CDF-S XT1 and XT2: White Dwarf Tidal Disruption Events by Intermediate-mass Black Holes?. Recently, two fast X-ray transients (XT1 and XT2) have been reported from the search in the Chandra Deep Field (CDF) data. Each transient shows an initial plateau lasting around hundreds to thousands of seconds followed by a rapid... | [
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Detection of Phosphorus-bearing Molecules toward a Solar-type Protostar. Phosphorus is a key ingredient in terrestrial biochemistry, but is rarely observed in the molecular interstellar medium and therefore little is known about how it is inherited during the star and planet formation sequence. We present observations ... | [
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Puffy Accretion Disks: Sub-Eddington, Optically Thick, and Stable. We report on a new class of solutions of black hole accretion disks that we have found through three-dimensional, global, radiative magnetohydrodynamic simulations in general relativity. It combines features of the canonical thin, slim, and thick disk m... | [
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A New Type of Jet in a Polar Limb of the Solar Coronal Hole. A new type of chromospheric jet in a polar limb of a coronal hole is discovered in the Ca II filtergram of the Solar Optical Telescope on board the Hinode. We identify 30 jets in a filtered Ca II movie with a duration of 53 minutes. The average speed at their... | [
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Comet C/2017 S3 (PanSTARRS): Outbursts and Disintegration. The Solar Wind ANisotropies (SWAN) all-sky hydrogen Lyα camera on the SOlar and Heliospheric Observer satellite observed the hydrogen coma of comet C/2017 S3 (PanSTARRS) for the last month of its activity from 2018 July 4 to August 4 and what appears to have be... | [
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Magnetohydrodynamic Seismology of Quiet Solar Active Regions. The ubiquity of recently discovered low-amplitude decayless kink oscillations of plasma loops allows for the seismological probing of the corona on a regular basis. In particular, in contrast to traditionally applied seismology that is based on the large-amp... | [
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An Ideal Testbed for Planet-Disk Interaction: Two Giant Protoplanets in Resonance Shaping the PDS 70 Protoplanetary Disk. While numerical simulations have been playing a key role in the studies of planet-disk interaction, testing numerical results against observations has been limited so far. With the two directly imag... | [
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Rapid Escape of Ultra-hot Exoplanet Atmospheres Driven by Hydrogen Balmer Absorption. Atmospheric escape is key to explaining the long-term evolution of planets in our solar system and beyond, and in the interpretation of atmospheric measurements. Hydrodynamic escape is generally thought to be driven by the flux of ext... | [
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Fast Extragalactic X-Ray Transients from Gamma-Ray Bursts Viewed Far Off-axis. The observed light curves and estimated sky rate of fast extragalactic X-ray transients (XRTs) discovered in archival Chandra data indicate that they belong to two distinct XRT populations. The first population of relatively short duration p... | [
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Quantifying the Effect of Black Hole Feedback from the Central Galaxy on the Satellite Populations of Groups and Clusters. Supermassive black holes are fundamental ingredients in our theoretical understanding of galaxy formation. They are likely the only sources energetic enough to regulate star formation within massiv... | [
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No Snowball on Habitable Tidally Locked Planets with a Dynamic Ocean. Terrestrial planets orbiting within the habitable zones of M-stars are likely to become tidally locked in a 1:1 spin:orbit configuration and are prime targets for future characterization efforts. An issue of importance for the potential habitability ... | [
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Signatures of a Planet-Planet Impacts Phase in Exoplanetary Systems Hosting Giant Planets. Exoplanetary systems host giant planets on substantially noncircular, close-in orbits. We propose that these eccentricities arise in a phase of giant impacts, analogous to the final stage of solar system assembly that formed Eart... | [
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Vapor Drainage in the Protolunar Disk as the Cause for the Depletion in Volatile Elements of the Moon. Lunar rocks are severely depleted in moderately volatile elements (MVEs) such as Rb, K, and Zn relative to Earth. Identifying the cause of this depletion is important for understanding how the Earth-Moon system evolve... | [
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Investigating Particle Acceleration in the Wolf-Rayet Bubble G2.4+1.4. The supersonic winds produced by massive stars carry a large amount of kinetic power. In numerous scenarios such winds have been proven to produce shocks in which relativistic particles are accelerated emitting nonthermal (NT) radiation. Here, we re... | [
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Ram-pressure Stripping of a Kicked Hill Sphere: Prompt Electromagnetic Emission from the Merger of Stellar Mass Black Holes in an AGN Accretion Disk. Accretion disks around supermassive black holes (SMBHs) are promising sites for stellar mass black hole (BH) mergers due to mass segregation and merger acceleration by di... | [
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Nearly all Massive Quiescent Disk Galaxies Have a Surprisingly Large Atomic Gas Reservoir. The massive galaxy population above the characteristic Schechter mass M * ≈ 1010.6 {M}⊙ contributes to about half of the total stellar mass in the local universe. These massive galaxies usually reside in hot dark matter halos ab... | [
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Parallel-propagating Fluctuations at Proton-kinetic Scales in the Solar Wind Are Dominated By Kinetic Instabilities. We use magnetic helicity to characterize solar wind fluctuations at proton-kinetic scales from Wind observations. For the first time, we separate the contributions to helicity from fluctuations propagati... | [
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An Improved Treatment of Neutral Sheet Drift in the Inner Heliosphere. Drifts due to the curvature and gradients in the heliospheric magnetic field, as well as along the heliospheric current sheet, have long been known to play a significant role in the transport of galactic cosmic rays. Recently, there has been greater... | [
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A Galaxy-targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan. On 2019 August 14 the Laser Interferometer Gravitational Wave Observatory (LIGO) and the Virgo gravitational wave interferometer announced the detection of a binary merger, S190814bv, with a low false alarm rate ... | [
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Spiral Structure in the Gas Disk of TW Hya. We report the detection of spiral substructure in both the gas velocity and temperature structure of the disk around TW Hya, suggestive of planet-disk interactions with an unseen planet. Perturbations from Keplerian rotation tracing out a spiral pattern are observed in the SE... | [
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Reynolds Number and Intermittency in the Expanding Solar Wind: Predictions Based on Voyager Observations. The large-scale features of the solar wind are examined in order to predict small-scale features of turbulence in unexplored regions of the heliosphere. The strategy is to examine how system size, or effective Reyn... | [
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Populations of Stellar-mass Black Holes from Binary Systems. In large and complicated stellar systems like galaxies, it is difficult to predict the number and characteristics of a black hole (BH) population. Such populations may be modeled as an aggregation of homogeneous (i.e., having uniform star formation history an... | [
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Probing the Survival of Planetary Systems in Globular Clusters with Tidal Disruption Events. Among the growing list of confirmed exoplanets, the number of planets identified in dense star clusters remains sparse. Previous analyses have suggested that this may be due in part to dynamical interactions that can unbind pla... | [
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Dynamical Masses for the Triple System HD 28363 in the Hyades Cluster. The star HD 28363 in the Hyades cluster has been known for over a century as a visual binary with a period of 40 yr. The secondary is, in turn, a single-lined spectroscopic binary with a 21 day period. Here we report extensive spectroscopic monitori... | [
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Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. II. Influence of Shock-surfing Acceleration on Downstream Electron Spectra. We explore electron preacceleration at high-Mach-number nonrelativistic perpendicular shocks at, e.g., young supernova remnants, which are a prerequisite o... | [
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Steepening of Cosmic-Ray Spectra in Shocks with Varying Magnetic Field Direction. Cosmic-ray (CR) spectra, both measured upon their arrival at the Earth’s atmosphere and inferred from the emission in supernova remnants (SNRs), appear to be significantly steeper than the “standard” diffusive shock acceleration (DSA) the... | [
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An Evolving Broad Iron Line from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124. We present a spectral study of the ultraluminous Be/X-ray transient pulsar Swift J0243.6+6124 using Neutron Star Interior Composition Explorer (NICER) observations during the system’s 2017-2018 giant outburst. The 1.2-10 ... | [
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Molecular Cloud Distances Based on the MWISP CO Survey and Gaia DR2. We present a new method of calculating distances of molecular clouds in the Galactic plane, using CO observations and the Gaia DR2 parallax and G-band extinction (A G ) measurements. Due to the complexity of dust environments in the Galactic plane, A... | [
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Thermodynamic Properties of Mirror Structures in the Magnetosheath: MMS Observations and Double-polytropic MHD Simulations. Mirror structures are manifested as a wave train of magnetic peaks and/or dips, which are anticorrelated with plasma density. The evolution behavior of the ion temperatures perpendicular and paral... | [
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Stages of Reionization as Revealed by the Minkowski Functionals. We study the evolution of the hydrogen ionization field during the epoch of reionization (EoR) using seminumerical simulations. By calculating the Minkowski functionals (MFs) of the 21 cm brightness temperature field, which provides a quantitative descrip... | [
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Tidal Disruption Events, Main-sequence Extreme-mass Ratio Inspirals, and Binary Star Disruptions in Galactic Nuclei. The Galactic Center has been under intense scrutiny in recent years thanks to pioneering missions aiming to measure the gas and star dynamics near the supermassive black hole (SMBH) and to find the gravi... | [
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Effects of ϕ-meson on the EOS, Maximum Masses, and Radii of Hyperon Stars. The relativistic mean field (RMF) model is considered as one of the best methods to study the nuclear system that has a high degree of isospin asymmetry and baryon density. In the present contribution, we take 25 well-known parameter sets of the... | [
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Structural and Evolutionary Diagnostics from Asteroseismic Phase Functions. In the asymptotic parameterization of mode frequencies, the phase function ∊(ν) completely specifies the detailed structure of the frequency eigenvalues. In practice, however, this function of frequency is reduced to a single scalar ∊, defined,... | [
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Evolutionary Models for R Coronae Borealis Stars. We use Modules for Experiments in Stellar Astrophysics (MESA) to construct stellar evolution models that reach a hydrogen-deficient, carbon-rich giant phase like the R Coronae Borealis (R CrB) stars. These models use opacities from OPAL and ÆSOPUS that cover the conditi... | [
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Integrated Spectra of Milky Way Globular Clusters. Integrated spectra of Milky Way globular clusters (GCs) are reproduced by computing synthetic spectra taking into account individual element abundances. Five clusters were selected from their location in the Galactic bulge, for which integrated spectra were available i... | [
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TESS Asteroseismology of the Known Red-giant Host Stars HD 212771 and HD 203949. The Transiting Exoplanet Survey Satellite (TESS) is performing a near all-sky survey for planets that transit bright stars. In addition, its excellent photometric precision enables asteroseismology of solar-type and red-giant stars, which ... | [
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CLOVER: Convnet Line-fitting Of Velocities in Emission-line Regions. When multiple star-forming gas structures overlap along the line of sight and emit optically thin emission at significantly different radial velocities, the emission can become non-Gaussian and often exhibits two distinct peaks. Traditional line-fitti... | [
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Further Evidence for Looplike Fine Structure inside “Unipolar” Active Region Plages. Earlier studies using extreme-ultraviolet images and line-of-sight magnetograms from the Solar Dynamics Observatory (SDO) have suggested that active region (AR) plages and strong network concentrations often have small, looplike featur... | [
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Ensemble Forecasting of Major Solar Flares with Short-, Mid-, and Long-term Active Region Properties. We apply an ensemble technique for major flare prediction by considering short-, mid-, and long-term active region (AR) properties and their relative contributions. For this, we consider magnetic parameters from Solar ... | [
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The Equation of State and Some Key Parameters of Neutron Stars: Constraints from GW170817, the Nuclear Data, and the Low-mass X-Ray Binary Data. In this work we parameterize the equation of state of dense neutron star (NS) matter with four pressure parameters of \{{\hat{p}}1,{\hat{p}}2,{\hat{p}}3,{\hat{p}}4\} and then ... | [
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Understanding Lyα Nebulae at Low Redshift. I. The Sizes, Powering, and Kinematics of “Green Bean” Galaxies. A new but rare sample of spatially extended emission line nebulae, nicknamed “Green Beans,” was discovered at z ≈ 0.3 thanks to strong [O III] emission, and subsequently shown to be local cousins of the Lyα nebul... | [
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SN 2017gmr: An Energetic Type II-P Supernova with Asymmetries. We present high-cadence UV, optical, and near-infrared data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days. SN 2017gmr does not show signs of narrow, high-ionization emission lines in the early optical s... | [
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The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar. We analyze extensive spectroscopic and photometric data of the hypervariable quasar SDSS J141324+530527 (RMID 017) at z = 0.456, an optical “changing-look” quasar from the Sloan Digital Sky... | [
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KIC 4142768: An Evolved Gamma Doradus/Delta Scuti Hybrid Pulsating Eclipsing Binary with Tidally Excited Oscillations. We present the characterization of KIC 4142768, an eclipsing binary with two evolved A-type stars in an eccentric orbit with a period of 14 days. We measure the fundamental parameters of the two compon... | [
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Cosmological Evolution of the Absorption of γ-Ray Burst X-Ray Afterglows. X-ray absorption of γ-ray burst (GRB) afterglows is prevalent yet poorly understood. X-ray-derived neutral hydrogen column densities (N H) of GRB X-ray afterglows show an increase with redshift, which might give a clue for the origin of this abso... | [
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Characterizing the Magnetic Environment of Exoplanet Stellar Systems. We employ a flux transport model incorporating observed stellar activity relations to characterize stellar interplanetary fields on cycle timescales for a range of stellar activity defined by the Rossby number. This framework allows us to examine the... | [
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Unveiling Dust Aggregate Structure in Protoplanetary Disks by Millimeter-wave Scattering Polarization. Dust coagulation in a protoplanetary disk is the first step in planetesimal formation. However, the pathway from dust aggregates to planetesimals remains unclear. Both numerical simulations and laboratory experiments ... | [
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Signatures of Tidal Disruption in Ultra-faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V. The ultra-faint dwarf galaxy Leo V has shown both photometric overdensities and kinematic members at large radii, along with a tentative kinematic gradient, suggesting that it may have undergone a clo... | [
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A Search for Short-term Hard X-Ray Bursts in the Direction of the Repeating FRB 121102. The nature of fast radio bursts (FRBs), which occur on millisecond timescales in the radio band, is well-understood. Among their unknown observational properties are their broadband spectra, and persistent and transient multiwavelen... | [
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A New Technique for Finding Galaxies Leaking Lyman-continuum Radiation: [S II]-deficiency. The source responsible for the reionization of the universe is believed to be the population of star-forming galaxies at z ∼ 6 to 12. The biggest uncertainty concerns the fraction of Lyman-continuum photons that actually escape f... | [
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Fast-to-Alfvén Mode Conversion and Ambipolar Heating in Structured Media. I. Simplified Cold Plasma Model. Linear fast magnetoacoustic waves are introduced into a cold stratified plasma model made up of a doubly periodic ensemble of straight diminished-Alfvén-speed tubes. Coupling between fast and Alfvén waves is produ... | [
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The Nature of Class I Sources: Periodic Variables in Orion. We present a quantitative, empirically based argument that at least some Class I sources are low-mass, pre-main-sequence stars surrounded by spatially extended envelopes of dusty gas. The source luminosity arises principally from stellar gravitational contract... | [
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The MOSDEF Survey: The Metallicity Dependence of X-Ray Binary Populations at z ∼ 2. Population synthesis models predict that high-mass X-ray binary (HMXB) populations produced in low-metallicity environments should be more X-ray luminous, a trend supported by studies of nearby galaxies. This trend may be responsible fo... | [
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Global 3D Hydrodynamic Modeling of In-transit Lyα Absorption of GJ 436b. Using a global 3D, fully self-consistent, multifluid hydrodynamic model, we simulate the escaping upper atmosphere of the warm Neptune GJ 436b, driven by the stellar X-ray and ultraviolet (XUV) radiation impact and gravitational forces and interac... | [
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2 mm GISMO Observations of the Galactic Center. I. Dust Emission. The central molecular zone, covering the inner ∼1° of the Galactic plane has been mapped at 2 mm using the Goddard-IRAM Superconducting 2-Millimeter Observer (GISMO) bolometric camera on the 30 m IRAM telescope. The 21″ resolution maps show abundant emis... | [
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2 mm GISMO Observations of the Galactic Center. II. A Nonthermal Filament in the Radio Arc and Compact Sources. We have used the Goddard IRAM 2 Millimeter Observer (GISMO) with the 30 m IRAM telescope to carry out a 2 mm survey of the Galaxy’s central molecular zone. These observations detect thermal emission from cold... | [
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Analysis of Helium-rich White Dwarfs Polluted by Heavy Elements in the Gaia Era. We present an analysis of 1023 DBZ/DZ(A) and 319 DQ white dwarf stars taken from the Montreal White Dwarf Database. This represents a significant increase over the previous comprehensive studies on these types of objects. We use new trigon... | [
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The Polarization Behavior of Relativistic Synchrotron Self-Compton Jets. We describe a geometric model for synchrotron and synchrotron self-Compton (SSC) radiation from blazar jets, involving multiple emission zones with turbulent magnetic fields and fully self-consistent seed photon mixing for SSC. Including the effec... | [
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Simulated Interactions between Radio Galaxies and Cluster Shocks. II. Jet Axes Orthogonal to Shock Normals. We report a 3D MHD simulation study of the interactions between radio galaxies (RGs) and galaxy-cluster-media shocks in which the incident shock normals are orthogonal to the bipolar active galactic nucleus (AGN)... | [
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Evolution of the Three-dimensional Shape of Passively Evolving and Star-forming Galaxies at z < 1. Using the HST/ACS I F814W-band data, we investigated the distribution of apparent axial ratios of ∼21,000 galaxies with M V < -20 at 0.2 < z < 1.0 in the COSMOS field as a function of stellar mass, specific ... | [
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The Central Star of NGC 2346 as a Clue to Binary Evolution through the Common Envelope Phase. We present an analysis of the binary central star of the planetary nebula NGC 2346 based on archival data from the International Ultraviolet Explorer, and new low- and high-resolution optical spectra (3700-7300 Å). By includin... | [
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Hβ and Hγ Absorption-line Profile Inconsistencies in Laboratory Experiments Performed at White Dwarf Photosphere Conditions. The spectroscopic method relies on hydrogen Balmer absorption lines to infer white dwarf (WD) masses. These masses depend on the choice of atmosphere model, hydrogen atomic line shape calculation... | [
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The Imprint of Spiral Arms on the Galactic Rotation Curve. We discuss a model for the Milky Way obtained by fitting the observed terminal velocities with the radial acceleration relation. The resulting stellar surface density profile departs from a smooth exponential disk, having bumps and wiggles that correspond to ma... | [
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Finding the Critical Decay Index in Solar Prominence Eruptions. The background field is assumed to play a prime role in erupting structures like prominences. In the flux rope models, the critical decay index (n c ) is a measure of the rate at which background field intensity decreases with height over the flux rope or... | [
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Solar Fast-drifting Radio Bursts in an X1.3 Flare on 2014 April 25. One of the most important products of solar flares is nonthermal energetic particles, which may carry up to 50% of the energy released in the flaring processes. In radio observations, nonthermal particles generally manifest as spectral fine structures ... | [
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Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet. Dust growth is often neglected when building models of protoplanetary disks due to its complexity and computational expense. However, it does play a major role in shaping the evolution of ... | [
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Multiscale Time- and Frequency-domain Likelihood Analysis with Photon Weights. We present an unbinned likelihood analysis formalism employing photon weights—the probabilities that events are associated with a particular source. This approach is applicable to any photon-resolving instrument and thus well suited to high-... | [
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Magnetospheric Accretion as a Source of Hα Emission from Protoplanets around PDS 70. Advances in high-resolution imaging have revealed Hα emission separate from the host star. It is generally believed that the emission is associated with planets forming in protoplanetary disks. However, the nature of this emission is s... | [
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Possible Contribution of Magnetized White Dwarf Binaries to Type Ia Supernova Populations. The evolution of an accreting white dwarf (WD) with a strong magnetic field toward a Type Ia supernova (SN Ia) may differ from the classical single-degenerate (SD) channel. In this paper, we perform binary population synthesis si... | [
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The Initial Physical Conditions of the Orion BN/KL Fingers. Orion BN/KL is an example of a poorly understood phenomena in star-forming regions involving the close encounters of young stellar objects. The explosive structure, the great variety of molecules observed, the energy involved in the event, and the mass of the ... | [
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Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur Revisited. We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton observations revealed an X-ray “blob” near the IR arc tracing the bow shock, possibly a no... | [
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Searching for the Magnetized Tidal Dwarf Galaxies in Hickson Compact Groups: HCG 26, 91, and 96. In this work, archive 1.4 and 4.86 GHz radio continuum data from the Very Large Array were re-reduced and, together with the 1.4 GHz maps from the NRAO VLA Sky Survey, investigated for the presence of detectable, nonthermal... | [
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Evidence for a Massive Warm-Hot Circumgalactic Medium around NGC 3221. We report a 3.4σ detection of the warm-hot, massive, extended circumgalactic medium (CGM) around an L ⋆ star-forming spiral galaxy NGC 3221, using deep Suzaku observations. The temperature of the gas is 106.1 K, comparable to that of the Milky Way C... | [
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"http://astrothesaurus.org/uat/752",
"http://astrothesaurus.org/uat/506",
"http://astrothesaurus.org/uat/384"
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Chemical Abundances in a Turbulent Medium-H<SUB>2</SUB>, OH<SUP>+</SUP>, H<SUB>2</SUB>O<SUP>+</SUP>, ArH<SUP>+</SUP>. Supersonic turbulence results in strong density fluctuations in the interstellar medium (ISM), which have a profound effect on the chemical structure. Particularly useful probes of the diffuse ISM are t... | [
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An Unusual Mid-infrared Flare in a Type 2 AGN: An Obscured Turning-on AGN or Tidal Disruption Event?. We report the discovery of an exceptional MIR flare in a Type 2 AGN, SDSS J165726.81+234528.1, at z = 0.059. This object brightened by 3 mag in the Wide-field Infrared Survey Explorer (WISE) W1 and W2 bands between 201... | [
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A BCG with Offset Cooling: Is the AGN Feedback Cycle Broken in A2495?. We present a combined radio/X-ray analysis of the poorly studied galaxy cluster A2495 (z = 0.07923) based on new EVLA and Chandra data. We also analyze and discuss Hα emission and optical continuum data retrieved from the literature. We find an offs... | [
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"http://astrothesaurus.org/uat/2005",
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Mass Loss on the Red Giant Branch: Plasmoid-driven Winds above the RGB Bump. The onset of cool massive winds in evolved giants is correlated with an evolutionary feature on the red giant branch (RGB) known as the “bump.” Also at the bump, shear instability in the star leads to magnetic fields that occur preferentially ... | [
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"http://astrothesaurus.org/uat/1634",
"http://astrothesaurus.org/uat/1693"
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Abundant Refractory Sulfur in Protoplanetary Disks. Sulfur is one of the most abundant elements in the universe, with important roles in astro-, geo-, and biochemistry. Its main reservoirs in planet-forming disks have previously eluded detection: gaseous molecules only account for <1% of total elemental sulfur, with... | [
"http://astrothesaurus.org/uat/1037",
"http://astrothesaurus.org/uat/75",
"http://astrothesaurus.org/uat/1300",
"http://astrothesaurus.org/uat/226",
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"http://astrothesaurus.org/uat/1634",
"http://astrothesaurus.org/uat/1911"
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Determining Fireball Fates Using the α-β Criterion. As fireball networks grow, the number of events observed becomes unfeasible to manage by manual efforts. Reducing and analyzing big data requires automated data pipelines. Triangulation of a fireball trajectory can swiftly provide information on positions and, with ti... | [
"http://astrothesaurus.org/uat/538",
"http://astrothesaurus.org/uat/1041",
"http://astrothesaurus.org/uat/1040",
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Dissecting the Hot Bubbles in LMC-N57 with XMM-Newton. We present a study of the diffuse X-ray emission from the star-forming region LMC-N 57 in the Large Magellanic Cloud. We use archival XMM-Newton observations to unveil in detail the distribution of hot bubbles in this complex. X-ray emission is detected from the ce... | [
"http://astrothesaurus.org/uat/1810",
"http://astrothesaurus.org/uat/848",
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