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The Generalized Ion-sound Speed in Space and Astrophysical Plasmas. A generalized ion-sound speed for space and astrophysical plasmas in the regions of near- and far-from-thermal equilibrium is derived in the context of the new formulated invariant Kappa distribution. Inspired by the recent studies on the origin of pol... | [
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Nonthermal Motions in a Polar Coronal Hole Measured with Hinode/EIS during an on-Orbit Partial Solar Eclipse on 2017 August 21. We have performed a spectroscopic observation over the south polar coronal hole (PCH) with the Hinode Extreme-ultraviolet (EUV) Imaging Spectrometer (EIS) during an on-orbit partial solar ecli... | [
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Anisotropic Mass Segregation in Rotating Globular Clusters. We investigate the internal dynamics of anisotropic, rotating globular clusters with a multimass stellar population by performing new direct N-body simulations. In addition to the well-known radial mass segregation effect, where heavy stars and stellar remnant... | [
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The Structure of Solar Coronal Mass Ejections in the Extreme-ultraviolet Passbands. So far, most studies on the structure of coronal mass ejections (CMEs) are conducted through white-light coronagraphs, demonstrating that about one third of CMEs exhibit the typical three-part structure in the high corona (e.g., beyond ... | [
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Cosmological Constraints from the Redshift Dependence of the Alcock-Paczynski Effect: Fourier Space Analysis. The tomographic Alcock-Paczynski (AP) method utilizes the redshift evolution of the AP distortion to place constraints on cosmological parameters. In previous works, it was performed via the anisotropic two-poi... | [
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Gravitational Lens System PS J0147+4630 (Andromeda’s Parachute): Main Lensing Galaxy and Optical Variability of the Quasar Images. Because follow-up observations of quadruple gravitational lens systems are of extraordinary importance for astrophysics and cosmology, we present single-epoch optical spectra and r-band lig... | [
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On the Origin of SN 2016hil—A Type II Supernova in the Remote Outskirts of an Elliptical Host. Type II supernovae (SNe) stem from the core collapse of massive (>8 M ⊙) stars. Due to their short lifespan, we expect a very low rate of such events in elliptical hosts, where the star formation rate is low, and which are... | [
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Ensemble Average of Three-dimensional Minkowski Tensors of a Gaussian Random Field in Redshift Space. We present the ensemble expectation values for the translation-invariant, rank-2 Minkowski tensors in three dimensions, for a linearly redshift-space-distorted Gaussian random field. The Minkowski tensors {W}10,2, {W}2... | [
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Morphological Classification of G-band Bright Points Based on Deep Learning. The G-band bright points (GBPs) are driven by the granular convection flow, and appear with different morphologies in the quiet Sun, such as points, elongated chains, and knees. A point-like GBP represents a single slender flux tube, while the... | [
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Formation and Eruption of a Mini-sigmoid Originating in Coronal Hole. In this paper, we study in detail the evolution of a mini-sigmiod originating in a cross-equatorial coronal hole, where the magnetic field is mostly open and seriously distinct from the closed background field above active-region sigmoids. The source... | [
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A Remarkably Narrow RHESSI X-Ray Flare on 2011 September 25. The unusually narrow X-ray source imaged with the Ramaty High Energy Solar Spectroscopic Imager (RHESSI) during an impulsive spike lasting for ∼10 s during the Geostationary Operational Environmental Satellite C7.9 flare on 2011 September 25 (SOL2011-09-25T03... | [
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Modulation of Galactic Cosmic Rays from Helium to Nickel in the Inner Heliosphere. Galactic cosmic-ray (GCR) helium and heavier ions are important sources of space radiation, and their elemental spectra and composition can help us better understand the transport in both the galaxy and the heliosphere. A model based on ... | [
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Multi-wavelength Variability Signatures of Relativistic Shocks in Blazar Jets. Mildly relativistic shocks that are embedded in colliding magnetohydrodynamic flows are prime sites for relativistic particle acceleration and the production of strongly variable, polarized multi-wavelength emission from relativistic jet sou... | [
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Evaluating the Classification of Fermi BCUs from the 4FGL Catalog Using Machine Learning. The recently published fourth Fermi Large Area Telescope source catalog (4FGL) reports 5065 gamma-ray sources in terms of direct observational gamma-ray properties. Among the sources, the largest population is the active galactic ... | [
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Active Galactic Nuclei with Ultrafast Outflows Monitoring Project: The Broad-line Region of Mrk 79 as a Disk Wind. We developed a spectroscopic monitoring project to investigate the kinematics of the broad-line region (BLR) in active galactic nuclei (AGNs) with ultrafast outflows (UFOs). Mrk 79 is a radio-quiet AGN wit... | [
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Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen. Recent analyses of 21 cm neutral hydrogen (H I) emission have demonstrated that H I gas is organized into linear filamentary structures that are preferentially aligned with the local magnetic field, and that the cohere... | [
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Critical Velocity Ionization in Substellar Atmospheres. The observation of radio, X-ray, and H α emission from substellar objects indicates the presence of plasma regions and associated high-energy processes in their surrounding envelopes. This paper numerically simulates and characterizes critical velocity ionization... | [
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Origin of Nonaxisymmetric Features of Virgo Cluster Early-type Dwarf Galaxies. II. Tidal Effects on Disk Features and Stability. A fraction of dwarf galaxies in the Virgo Cluster contain disk features like bars and spiral arms. Using N-body simulations, we investigate the effects of tidal forces on the formation of suc... | [
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Measuring and Modeling the Rate of Separator Reconnection between an Emerging and an Existing Active Region. Magnetic reconnection occurs when new flux emerges into the corona and becomes incorporated into the existing coronal field. A new active region (AR) emerging in the vicinity of an existing AR provides a conveni... | [
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First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7. The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to perform sky-model and redundant interferometric calibrati... | [
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A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments. Line intensity mapping (LIM) is a promising approach to study star formation and the interstellar medium (ISM) in galaxies by measuring the aggregate line emission from the entire galaxy population. In this work, we develop a simp... | [
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ALMA Observations of Atomic Carbon [C I] ( <SUP> 3 </SUP> P <SUB> 1 </SUB> → <SUP> 3 </SUP> P <SUB> 0 </SUB>) and Low-J CO Lines in the Starburst Galaxy NGC 1808. We present [C I] ≤ft({}3{{P}}1\to {}3{{P}}0\right), 12CO, 13CO, and C18O (J=2\to 1) observations of the central region (radius 1 kpc) of the starburst galaxy... | [
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Discovery of Four Apparently Cold Dusty Galaxies at z = 3.62-5.85 in the COSMOS Field: Direct Evidence of Cosmic Microwave Background Impact on High-redshift Galaxy Observables. We report Atacama Large Millimeter Array (ALMA) observations of four high-redshift dusty star-forming galaxy candidates selected from far-infr... | [
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Generic Regular Black Holes Related to Nonlinear Electrodynamics with Maxwellian Weak-field Limit: Shadows and Images of Keplerian Disks. We study optical phenomena in generic regular, magnetically charged, spherically symmetric black hole spacetimes arising from coupling of the Einstein gravity and nonlinear electrody... | [
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Active Region Modulation of Coronal Hole Solar Wind. Active regions (ARs) are a candidate source of the slow solar wind (SW), the origins of which are a topic of ongoing research. We present a case study that examines the processes by which SW is modulated in the presence of an AR in the vicinity of the SW source. We c... | [
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Kinematics of the M87 Jet in the Collimation Zone: Gradual Acceleration and Velocity Stratification. We study the kinematics of the M87 jet using the first-year data of the KVN and VERA Array (KaVA) large program, which has densely monitored the jet at 22 and 43 GHz since 2016. We find that the apparent jet speeds gene... | [
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The Canada-France Imaging Survey: Reconstructing the Milky Way Star Formation History from Its White Dwarf Population. As the remnants of stars with initial masses ≲8 M ⊙, white dwarfs contain valuable information on the formation histories of stellar populations. In this paper, we use deep, high-quality, u-band photom... | [
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Origins of Molecular Clouds in Early-type Galaxies. We analyze Chandra observations of the hot atmospheres of 40 early spiral and elliptical galaxies. Using new temperature, density, cooling time, and mass profiles, we explore relationships between their hot atmospheres and cold molecular gas. Molecular gas mass correl... | [
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Numerical Simulation on the Propagation and Deflection of Fast Coronal Mass Ejections (CMEs) Interacting with a Corotating Interaction Region in Interplanetary Space. Previous research has shown that the deflection of coronal mass ejections (CMEs) in interplanetary space, especially fast CMEs, is a common phenomenon. T... | [
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Camouflage of the Phase Transition to Quark Matter in Neutron Stars. It has been known for some time that compact stars containing quark matter can masquerade as neutron stars in the range of measured mass and radius, making it difficult to draw firm conclusions on the phases of matter present inside the star. Using th... | [
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Circumplanetary Disk Dynamics in the Isothermal and Adiabatic Limits. Circumplanetary disks (CPDs) may be essential to the formation of planets, regulating their spin and accretion evolution. We perform a series of 3D hydrodynamics simulations in both the isothermal and adiabatic limits to systematically measure the ro... | [
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Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters. We investigate constraints on some key cosmological parameters by confronting metastable dark energy (DE) models with different combinations of the most recent cosmological observations. Along with the standard ΛCDM model, two ... | [
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Spectroscopic and Stereoscopic Observations of the Solar Jets. We present a comprehensive study of a series of recurrent jets that occurred at the periphery of the NOAA active region 12114 on 2014 July 7. These jets were found to share the same source region and exhibited rotational motions as they propagated outward. ... | [
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GASP XXIII: A Jellyfish Galaxy as an Astrophysical Laboratory of the Baryonic Cycle. With MUSE, Chandra, VLA, ALMA, and UVIT data from the GASP program, we study the multiphase baryonic components in a jellyfish galaxy (JW100) with a stellar mass 3.2 × 1011 M ☉ hosting an active galactic nucleus (AGN). We present its s... | [
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Spectral Evolution and Radial Dust Transport in the Prototype Young Eruptive System EX Lup. EX Lup is the prototype of a class of pre-main-sequence eruptive stars defined by their repetitive outbursts lasting several months. In 2008 January-September EX Lup underwent its historically largest outburst, brightening by ab... | [
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The Exoplanet Population Observation Simulator. II. Population Synthesis in the Era of Kepler. The collection of planetary system properties derived from large surveys such as Kepler provides critical constraints on planet formation and evolution. These constraints can only be applied to planet formation models, howeve... | [
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Jellyfish: Resolving the Kinematics of Extreme Ram-pressure Stripping at z ∼ 0.3. We present and discuss results from the first spatially resolved kinematic study of ram-pressure stripping of a massive late-type galaxy at intermediate redshifts. Our target, the spectacular “jellyfish” galaxy, A1758N_JFG1, was previousl... | [
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An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission. It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree of polarization depends on the angle ψ between the interstellar magnetic field and the line of sight (LOS). However, anisotropy of the du... | [
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No Evidence for Critical Balance in Field-aligned Alfvénic Solar Wind Turbulence. The properties of Alfvénic solar wind turbulence have been studied for decades using spacecraft measurements. In particular, the observation of spectral anisotropy of magnetic fluctuations has stimulated the development of several phenome... | [
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Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization. Outflows are a pervasive feature of mechanical feedback from super star clusters (SSCs) in starburst galaxies, playing a fundamental role in galaxy evolution. Observations are now starting to confirm that outflows can undergo catastrophic... | [
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Testing Cosmic Opacity with the Combination of Strongly Lensed and Unlensed Supernova Ia. In this paper, we present a scheme to investigate the opacity of the universe in a cosmological-model-independent way, with the combination of current and future measurements of an SN Ia sample and galactic-scale strong gravitatio... | [
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The Generalized Hardness-Intensity Diagram for Black Hole and Neutron Star X-Ray Binaries. Over the past half-century, X-ray and radio observations of accreting neutron stars and stellar-mass black holes have yielded a rich observational picture, with common features including state transitions and jet formation, but a... | [
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dHybridR: A Hybrid Particle-in-cell Code Including Relativistic Ion Dynamics. We present the first plasma simulations obtained with the code dHybridR, a hybrid particle-in-cell code with fluid electrons and both thermal and energetic ions that retain relativistic dynamics. dHybridR is constructed to study astrophysical... | [
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Information in the Reflected-light Spectra of Widely Separated Giant Exoplanets. Giant exoplanets located >1 au away from their parent stars have atmospheric environments cold enough for water or ammonia clouds. We have developed a new equilibrium cloud and reflected-light spectrum model, ExoREL, for widely separate... | [
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Radiative Properties of Magnetically Arrested Disks. Magnetically arrested disks (MADs) appear when accretion flows are supplied with a sufficient amount of magnetic flux. In this work, we use results of magnetohydrodynamic simulations to set the configuration of the magnetic field and investigate the dynamics and radi... | [
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The Detection of [O III] λ4363 in a Lensed, Dwarf Galaxy at z = 2.59: Testing Metallicity Indicators and Scaling Relations at High Redshift and Low Mass. We present Keck/MOSFIRE (Multi-Object Spectrometer for InfraRed Exploration) and Keck/LRIS (Low Resolution Imaging Spectrometer) spectroscopy of A1689-217, a lensed (... | [
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Transit Signatures of Inhomogeneous Clouds on Hot Jupiters: Insights from Microphysical Cloud Modeling. We determine the observability in transmission of inhomogeneous cloud cover on the limbs of hot Jupiters through post-processing a general circulation model to include cloud distributions computed using a cloud micro... | [
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X-Ray Observations of a z ∼ 6.2 Quasar/Galaxy Merger. Quasars at early redshifts (z > 6) with companion galaxies offer unique insights into the growth and evolution of the first supermassive black holes. Here, we report on a 150 ks Chandra observation of PSO J308.0416-21.2339, a z = 6.23 quasar with a merging compan... | [
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"http://astrothesaurus.org/uat/1821",
"http://astrothesaurus.org/uat/608"
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Estimating the Molecular Gas Mass of Low-redshift Galaxies from a Combination of Mid-infrared Luminosity and Optical Properties. We present CO (J = 1-0) and/or CO (J = 2-1) spectroscopy for 31 galaxies selected from the ongoing Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, obtained with multiple t... | [
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NuSTAR Uncovers an Extremely Local Compton-thick AGN in NGC 4968. We present the analysis of Chandra and NuSTAR spectra of NGC 4968, a local (D ∼ 44 Mpc) 12 μm selected Seyfert 2 galaxy, enshrouded within Compton-thick layers of obscuring gas. We find no evidence of variability between the Chandra and NuSTAR observatio... | [
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Submillimeter Signatures from Growing Supermassive Black Holes before Reionization. The presence of supermassive black holes (SMBHs) with masses up to M • ∼ 109 {M}⊙ at redshifts z ≃ 7.5 suggests that their seeds may have started to grow long before the reionization in ambient medium with pristine chemical composition... | [
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The Galaxy Power Spectrum from TGSS ADR1 and the Effect of Flux Calibration Systematics. We explore the large to moderate scale anisotropy in distant radio sources using the TIFR GMRT Sky Survey (TGSS) ADR1 catalog. We use different measures, i.e., number counts, sky brightness, and flux per source, for this study. In ... | [
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"http://astrothesaurus.org/uat/1464",
"http://astrothesaurus.org/uat/1671",
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Star-density Profiles of Six Old Star Clusters in the Large Magellanic Cloud. We used resolved star counts from Hubble Space Telescope (HST) images to determine the center of gravity and the projected density profiles of six old globular clusters (GCs) in the Large Magellanic Cloud (LMC), namely NGC 1466, NGC 1841, NGC... | [
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"http://astrothesaurus.org/uat/990",
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Electron Temperatures in the Dayside Ionosphere of Mars Derived from {{{\rm{O}}}_{2}}^{+} Chemistry. From a reduced chemical model of the Martian dayside ionosphere we derive an expression that can be used to estimate the electron temperature as a function of the ambient number densities of CO2, O, {{{{O}}}2}+, {CO}}2}... | [
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A Kinematic Shift of the C IV Broad Absorption Line in Quasar SDSS J120819.29+035559.4. We report the kinematic shift of the C IV broad absorption line (BAL) in quasar SDSS J120819.29+035559.4 (hereafter J1208+0355). This quasar shows two BAL systems, including a blue component of system A at ∼23,500 km s-1 that shows ... | [
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"http://astrothesaurus.org/uat/183",
"http://astrothesaurus.org/uat/1319"
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The Density Gradient Inside Molecular-gas Clumps as a Booster of Their Star Formation Activity. Star-forming regions presenting a density gradient experience a higher star formation rate than if they were of uniform density. We refer to the ratio between the star formation rate of a spherical centrally concentrated gas... | [
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The Progenitors of Calcium-strong Transients. A new class of faint, spectroscopically peculiar transients has emerged in the last decade. We term these events “calcium-strong transients” (CaSTs) because of their atypically high calcium-to-oxygen nebular line ratios. Previous studies have struggled to deduce the identit... | [
"http://astrothesaurus.org/uat/1799",
"http://astrothesaurus.org/uat/154",
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X-Ray Spectra from Plasmas with High-energy Electrons: κ-distributions and e<SUP>-</SUP>-e<SUP>-</SUP> Bremsstrahlung. Shocks, turbulence, and winds all influence the electron velocity distribution in hot plasmas, exciting lower-energy electrons and generating a high-energy (typically power-law) tail. This effect, typi... | [
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On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0-2.5. We present ALMA Band 6 (ν = 233 GHz, λ = 1.3 mm) continuum observations toward 68 “normal” star-forming galaxies within two Coma-like progenitor structures at z = 2.10 and 2.47, from which ISM... | [
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The Spin of the Black Hole GRS 1716-249 Determined from the Hard Intermediate State. We present three simultaneous/quasi-simultaneous NuSTAR and Swift data sets of the black hole (BH) GRS 1716-249 in its hard intermediate state. The accretion disk in this state may have reached the innermost stable circular orbit, and ... | [
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Long-term Variability and Correlation Study of the Blazar 3C 454.3 in the Radio, NIR, and Optical Wavebands. We performed a long-term optical (B, V, R bands), infrared (J and K bands), and radio band (15, 22, 37 GHz band) study of the flat spectrum radio quasar, 3C 454.3, using data collected over a period of more than... | [
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Synthetic Large-scale Galactic Filaments: On Their Formation, Physical Properties, and Resemblance to Observations. Using a population of large-scale filaments extracted from an AREPO simulation of a Milky Way-like galaxy, we seek to understand the extent to which observed large-scale filament properties (with lengths ... | [
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New s-process Mechanism in Rapidly Rotating Massive Population II Stars. We report a new mechanism for the s-process in rotating massive metal-poor stars. Our models show that above a critical rotation speed, such stars evolve in a quasi-chemically homogeneous fashion, which gives rise to a prolific s-process. Rotation... | [
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SN Ia Explosions from Hybrid Carbon-Oxygen-Neon White Dwarf Progenitors that Have Mixed during Cooling. The creation of “hybrid” white dwarfs, made of a C-O core within an O-Ne shell has been proposed, and studies indicate that ignition in the C-rich central region makes these viable progenitors for thermonuclear (type... | [
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Near L-edge Single and Multiple Photoionization of Triply Charged Iron Ions. Relative cross sections for m-fold photoionization (m = 1,…, 5) of Fe3+ by single-photon absorption were measured employing the photon-ion merged-beams setup PIPE at the PETRA III synchrotron light source operated at DESY in Hamburg, Germany. ... | [
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"http://astrothesaurus.org/uat/2073",
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Scattering of Energetic Electrons by Heat-flux-driven Whistlers in Flares. The scattering of electrons by heat-flux-driven whistler waves is explored with a particle-in-cell simulation relevant to the transport of energetic electrons in flares. This simulation is initiated with a large heat flux produced by using a kap... | [
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A Novel Energy-conserving Scheme for Eight-dimensional Hamiltonian Problems. We design a novel, exact energy-conserving implicit nonsymplectic integration method for an eight-dimensional Hamiltonian system with four degrees of freedom. In our algorithm, each partial derivative of the Hamiltonian with respect to one of ... | [
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Kinetic Helicity and Lifetime of Activity Complexes During Solar Cycle 24. We study magnetic features on the solar surface that exist for several rotations during solar cycle 24. To identify them, we average synoptic maps over a range in latitude and stack the resulting longitudinal strips in time. We use synoptic maps... | [
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Elemental Abundance Distributions in the (R, V <SUB> ϕ </SUB>) Plane with LAMOST DR5 and Gaia DR2. Since Gaia DR2 was released, many velocity structures in the disk have been revealed, such as large-scale ridge-like patterns in phase space. Both kinematic information and stellar elemental abundances are needed to revea... | [
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Impact of Clouds and Hazes on the Simulated JWST Transmission Spectra of Habitable Zone Planets in the TRAPPIST-1 System. The TRAPPIST-1 system, consisting of an ultracool host star having seven known Earth-sized planets, will be a prime target for atmospheric characterization with the James Webb Space Telescope (JWST)... | [
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A 40 Billion Solar-mass Black Hole in the Extreme Core of Holm 15A, the Central Galaxy of Abell 85. Holm 15A, the brightest cluster galaxy of the galaxy cluster Abell 85, has an ultradiffuse central region, ∼ 2 {mag} fainter than the faintest depleted core of any early-type galaxy (ETG) that has been dynamically modele... | [
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The REQUIEM Survey. I. A Search for Extended Lyα Nebular Emission Around 31 z > 5.7 Quasars. The discovery of quasars a few hundred megayears after the Big Bang represents a major challenge to our understanding of black holes as well as galaxy formation and evolution. Quasars' luminosity is produced by extreme gas a... | [
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Climates of Warm Earth-like Planets. III. Fractional Habitability from a Water Cycle Perspective. The habitable fraction of a planet’s surface is important for the detectability of surface biosignatures. The extent and distribution of habitable areas are influenced by external parameters that control the planet’s clima... | [
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Supernovae within Pre-existing Wind-blown Bubbles: Dust Injection versus Ambient Dust Destruction. By means of 3D hydrodynamical simulations, we evaluate here the impact that supernova (SN) explosions occurring within wind-driven bubbles have on the survival or destruction of dust grains. We consider both the dust gene... | [
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Combined Effects of Rotation and Age Spreads on Extended Main-Sequence Turn Offs. The extended main-sequence turn offs (eMSTOs) of several young to intermediate age clusters are examined in the Magellanic Clouds and the Milky Way. We explore the effects of extended star formation (eSF) and a range of stellar rotation r... | [
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A Dissection of Spatially Resolved AGN Feedback across the Electromagnetic Spectrum. We present optical SuperNova Integral Field Spectrograph integral field spectroscopy, Hubble Space Telescope optical imaging, Chandra X-ray imaging, and Very Large Array radio interferometry of the merging galaxy 2MASX J04234080+040801... | [
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On the Rapid Orbital Expansion in the Compact Low-mass X-Ray Binary 2A 1822-371. The neutron star (NS) low-mass X-ray binary 2A 1822-371 has an orbital period of 5.57 hr. Mass transfer in such short-period binaries is thought to be driven by magnetic braking with orbital shrinking. However, 2A 1822-371 shows a very rap... | [
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Consequences of Energetic Magnetar-like Outbursts of Nearby Neutron Stars: <SUP>14</SUP>C Events and the Cosmic Electron Spectrum. Four significant events of rapid 14C increase have taken place within the past several thousand years. The physical origin of these rapid increases is still a mystery but must be associated... | [
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Core-Envelope Coupling in Intermediate-mass Core-helium Burning Stars. Stars between two and three solar masses rotate rapidly on the main sequence, and the detection of slow core and surface rotation in the core-helium burning phase for these stars places strong constraints on their angular momentum transport and loss... | [
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Spatially Resolved Properties of Galaxies from CANDELS+MUSE: Radial Extinction Profile and Insights on Quenching. Studying the internal processes of individual galaxies at kilo-parsec scales is crucial in enhancing our understanding of galaxy formation and evolution processes. In this work, we investigate the distribut... | [
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Thermal State of the Intergalactic Medium at z ∼ 2-4. We present a new method to infer parameters of the temperature-density relation in the intergalactic medium in the post-reionization epoch at z ∼ 2-4. This method is based on the analysis of the distribution of Lyα absorbers over column densities and Doppler paramet... | [
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Deep ATCA and VLA Radio Observations of Short-GRB Host Galaxies. Constraints on Star Formation Rates, Afterglow Flux, and Kilonova Radio Flares. We report the results of an extensive radio-continuum observing campaign of host galaxies of short gamma-ray bursts (GRBs). The goal of this survey was to search for optically... | [
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The Contribution of Galaxies to the 3.4 μm Cosmic Infrared Background as Measured Using WISE. The study of the extragalactic background light (EBL) in the optical and near-infrared has received a lot of attention in the last decade, especially near the wavelength λ ≈ 3.4 μm, with remaining tension among different techn... | [
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Proton-Proton Collisions in the Turbulent Solar Wind: Hybrid Boltzmann-Maxwell Simulations. The mechanism of heating for hot, dilute, and turbulent plasmas represents a long-standing problem in space physics, whose implications concern both near-Earth environments and astrophysical systems. In order to explore the poss... | [
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Protostellar Evolution in Serpens Main: Possible Origin of Disk-size Diversity. We have observed the submillimeter continuum condensations SMM2, SMM4, SMM9, and SMM11 in the star-forming cluster Serpens Main using the Atacama Large Millimeter/submillimeter Array during Cycle 3 in the 1.3 mm continuum, 12CO J = 2 - 1, S... | [
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Impact of a Spinning Supermassive Black Hole on the Orbit and Gravitational Waves of a Nearby Compact Binary. Recent theoretical studies suggest that stellar-mass binary black holes (BBHs) would merge more efficiently due to the Kozai-Lidov (K-L) mechanism if these binaries form in the vicinity of supermassive black ho... | [
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Primordial Earth Mantle Heterogeneity Caused by the Moon-forming Giant Impact?. The giant impact hypothesis for Moon formation successfully explains the dynamic properties of the Earth-Moon system but remains challenged by the similarity of isotopic fingerprints of the terrestrial and lunar mantles. Moreover, recent ge... | [
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MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver. We present MAESTROeX, a massively parallel solver for low Mach number astrophysical flows. The underlying low Mach number equation set allows for efficient, long-time integration for highly subsonic flows compared to compressible approaches. MAESTROe... | [
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Stochastic Chemical Evolution of Radioactive Isotopes with a Monte Carlo Approach. Short-lived radionuclides (SLRs) with mean lives τ of a few to hundreds of Myr provide unique opportunities to probe recent nucleosynthesis events in the interstellar medium and the physical conditions in which the Sun formed. Here we qu... | [
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Planck Far-infrared Detection of Hyper Suprime-Cam Protoclusters at z ∼ 4: Hidden AGN and Star Formation Activity. We perform a stacking analysis of Planck, AKARI, Infrared Astronomical Satellite, Wide-field Infrared Survey Explorer, and Herschel images of the largest number of (candidate) protoclusters at z ∼ 3.8 sele... | [
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On the Origin of Solar Torsional Oscillations and Extended Solar Cycle. We present a nonlinear mean-field model of the solar interior dynamics and dynamo, which reproduces the observed cyclic variations of the global magnetic field of the Sun, as well as the differential rotation and meridional circulation. Using this ... | [
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Imaging the Sun's Far-side Active Regions by Applying Multiple Measurement Schemes on Multiskip Acoustic Waves. Being able to image active regions (ARs) on the Sun’s far side is useful for modeling the global-scale magnetic field around the Sun and for predicting the arrival of major ARs that rotate around the limb ont... | [
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Radiation Pressure from Interstellar Hydrogen Observed by IBEX through Solar Cycle 24. As the Sun moves through the local interstellar medium (LISM), neutral atoms travel through the heliosphere and can be detected by IBEX. We consider interstellar neutral (ISN) hydrogen atoms with a drifting Maxwellian distribution fu... | [
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The Spectral Evolution of AT 2018dyb and the Presence of Metal Lines in Tidal Disruption Events. We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg/AT 2018dyb spanning a period of one year. The event shows a plethora of strong emission lines, including the Balmer series, He II, He I, an... | [
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"http://astrothesaurus.org/uat/1911",
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Gamma-Ray Burst Host Galaxies: Specific Star Formation Rate versus Metallicity. The observed properties of long gamma-ray burst (GRB) host galaxies show them to often be of a rather low metallicity and/or of high specific star formation rate (SFR). It is not clear which of these properties is a dominant factor in deter... | [
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Recurrent Two-sided Loop Jets Caused By Magnetic Reconnection between Erupting Minifilaments and a nearby Large Filament. Using high spatial and temporal data from the New Vacuum Solar Telescope and the Solar Dynamics Observatory, we present unambiguous observations of recurrent two-sided loop jets caused by magnetic r... | [
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"http://astrothesaurus.org/uat/1495",
"http://astrothesaurus.org/uat/1503"
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Transition Region Loops in the Very Late Phase of Flux Emergence in IRIS Sit-and-stare Observations. Loops are one of the fundamental structures that trace the geometry of the magnetic field in the solar atmosphere. Their evolution and dynamics provide a crucial proxy for studying how the magnetized structures are form... | [
"http://astrothesaurus.org/uat/1477",
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"http://astrothesaurus.org/uat/1558",
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From Sun to Interplanetary Space: What is the Pathlength of Solar Energetic Particles?. Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar wind before being observed with in situ instruments. In order to interpret their origin through comparison with remote sensing observ... | [
"http://astrothesaurus.org/uat/1491",
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"http://astrothesaurus.org/uat/827",
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"http://astrothesaurus.org/uat/1534",
"http://astrothesaurus.org/uat/1693",
"http://astrothesaurus.org/uat/2191"
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