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Evolving LMXBs: CARB Magnetic Braking. The formation of low-mass X-ray binaries (LMXBs) is an ongoing challenge in stellar evolution. An important subset of LMXBs is the binary systems with a neutron star (NS) accretor. In NS LMXBs with nondegenerate donors, the mass transfer (MT) is mainly driven by magnetic braking (... | [
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MESSENGER Observations of Giant Plasmoids in Mercury’s Magnetotail. Small-scale flux ropes, with estimated diameters of ∼500 km and that pass over the MESSENGER spacecraft on timescales of seconds or less, are a common feature in Mercury’s magnetosphere. These magnetic structures, sometimes referred to as plasmoids, ar... | [
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Bright Gamma-Ray Flares Observed in GRB 131108A. GRB 131108A is a bright long gamma-ray burst (GRB) detected by the Large Area Telescope and the Gamma-ray Burst Monitor on board the Fermi Gamma-ray Space Telescope. Dedicated temporal and spectral analyses reveal three γ-ray flares dominating above 100 MeV, which are no... | [
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The Formation of CME from Coupling Fan-spine Magnetic System: A Difficult Journey. We present the eruption of a mini-filament that caused a large-scale complicated coronal mass ejection (CME) on 2014 March 28, using the high-resolution observations taken by the Solar Dynamic Observatory. Three-dimensional coronal magne... | [
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ALMA C II 158 μm Imaging of an H I-selected Major Merger at z ∼ 4. We present high spatial resolution (≈2 kpc) Atacama Large Millimeter/submillimeter Array (ALMA) observations of [C II] 158 μm and dust-continuum emission from a galaxy at z=3.7978 selected by its strong H I absorption (a damped Lyα absorber, DLA) agains... | [
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Laboratory Experiments on the Motion of Dense Dust Clouds in Protoplanetary Disks. In laboratory experiments, we study the motion of levitated, sedimenting clouds of submillimeter grains at low ambient pressure and at high solid-to-gas ratios ɛ. The experiments show a collective behavior of particles, i.e., grains in c... | [
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Frequency of Coronal Mass Ejection Impacts with Early Terrestrial Planets and Exoplanets around Active Solar-like Stars. Energetic flares and associated coronal mass ejections (CMEs) from young magnetically active solar-like stars can play a critical role in setting conditions for atmospheric escape as well as penetrat... | [
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Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Schwabe cycle of solar activity exhibits modulations and frequency fluctuations on slow timescales of centuries and millennia. Plausible physical explanations for the cause of these long-term variations of the solar cycle ar... | [
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High-frequency Wave Propagation Along a Spicule Observed by CLASP. The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) sounding rocket experiment, launched in 2015 September, observed the hydrogen Lyα line (121.6 nm) in an unprecedented high temporal cadence of 0.3 s. CLASP performed sit-and-stare observations of... | [
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A Statistical Approach to Planetesimal Condensate Composition beyond the Snowline Based on the Carbon-to-oxygen Ratio. The ratio between carbon and oxygen is regarded as an important driver of circumstellar and planetary chemistry, which can be used as a parameter to estimate the fractionation among refractory and vola... | [
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Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II Supernovae. We present 81 near-infrared (NIR) spectra of 30 Type II supernovae (SNe II) from the Carnegie Supernova Project-II (CSP-II), the largest such data set published to date. We identify a number of NIR features and characterize thei... | [
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The COS CGM Compendium. III. Metallicity and Physical Properties of the Cool Circumgalactic Medium at z ≲ 1. We characterize the metallicities and physical properties of cool, photoionized gas in a sample of 152 z ≲ 1 strong Lyα forest systems (SLFSs, absorbers with 15 < log N H I < 16.2). The sample is drawn fr... | [
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Isotopic Signatures of Supernova Nucleosynthesis in Presolar Silicon Carbide Grains of Type AB with Supersolar <SUP>14</SUP>N/<SUP>15</SUP>N Ratios. We report high-resolution C, N, Al, Si, and S isotope data of 38 presolar SiC grains of type AB. Seventeen of these grains are of subtype AB1 (14N/15N < 440 = solar) an... | [
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Inferring Galactic Parameters from Chemical Abundances: A Multi-star Approach. Constraining parameters such as the initial mass function high-mass slope and the frequency of Type Ia supernovae is of critical importance in the ongoing quest to understand galactic physics and create realistic hydrodynamical simulations. ... | [
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Revealing Hidden Substructures in the M <SUB>BH</SUB>-σ Diagram, and Refining the Bend in the L-σ Relation. Using 145 early- and late-type galaxies (ETGs and LTGs) with directly measured supermassive black hole masses, M BH, we build upon our previous discoveries that: (i) LTGs, most of which have been alleged to conta... | [
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Learning about the Intermediate Neutron-capture Process from Lead Abundances. Lead (Pb) is predominantly produced by the slow neutron-capture process (s process) in asymptotic giant branch (AGB) stars. In contrast to significantly enhanced Pb abundances predicted by low-mass, low-metallicity AGB models, observations of... | [
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Carbon-deficient Red Giants. Carbon-deficient red giants (CDRGs) are a rare class of peculiar red giants, also called “weak G-band” or “weak CH” stars. Their atmospheric compositions show depleted carbon, a low {}12{{C}}{/}13{{C}} isotopic ratio, and an overabundance of nitrogen, indicating that the material at the sur... | [
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Spectral Analysis of Fermi-LAT Gamma-Ray Bursts with Known Redshift and their Potential Use as Cosmological Standard Candles. Long duration gamma-ray bursts may serve as standard candles to constrain cosmological parameters by probing the Hubble diagram well beyond the range of redshift currently accessible using SNe I... | [
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Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Neutral Chlorine. We present lifetime measurements using beam-foil techniques for radiative transitions from the 3p 4(1 S)4s 2 S 1/2, 3p 4(3 P)5 {s}2{P}1/{2,3/2}, and 3p 4(3 P)3d 2 F 5/2 levels in Cl I and the corresponding results of the oscillator stre... | [
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Two New “Turn-off” Changing-look Active Galactic Nuclei and Implication on “Partially Obscured” AGNs. We report a spectroscopic identification of two new changing-look active galactic nuclei (CL-AGNs): SDSS J104705.16+544405.8 and SDSS J120447.91+170256.8, both with a “turn-off” type transition from type-1 to type-1.8/... | [
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On the Prospect of Using the Maximum Circular Velocity of Halos to Encapsulate Assembly Bias in the Galaxy-Halo Connection. We investigate a conceptual modification of the halo occupation distribution approach, using the halos’ present-day maximal circular velocity, V max, as an alternative to halo mass. In particular,... | [
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Classification of New X-Ray Counterparts for Fermi Unassociated Gamma-Ray Sources Using the Swift X-Ray Telescope. Approximately one-third of the gamma-ray sources in the third Fermi-LAT catalog are unidentified or unassociated with objects at other wavelengths. Observations with the X-Ray Telescope on the Neil Gehrels... | [
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Deep Chandra Survey of the Small Magellanic Cloud. III. Formation Efficiency of High-mass X-Ray Binaries. We have compiled the most complete census of high-mass X-ray binaries (HMXBs) in the Small Magellanic Cloud with the aim to investigate the formation efficiency of young accreting binaries in its low-metallicity en... | [
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Lorentz Factors of Compact Jets in Black Hole X-Ray Binaries. Compact, continuously launched jets in black hole X-ray binaries (BHXBs) produce radio to optical/IR synchrotron emission. In most BHXBs, an IR excess (above the disk component) is observed when the jet is present in the hard spectral state. We investigate w... | [
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A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). IV. The Submillimeter Properties of X-Ray Sources in the CDF-S. The Chandra Deep Field (CDF)-S is the deepest X-ray image available and will remain so for the near future. We provide a spectroscopic (64.5%; 64% with spectral classifications) and photometric... | [
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Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA. We present ALMA observations of the CO(1-0) line and 3 mm continuum emission in eight ultraluminous infrared (IR) quasi-stellar objects (QSOs) at z = 0.06-0.19. All eight IR QSO hosts are clearly resolved in their CO molecular gas emission... | [
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Shocked Narrow-angle Tail Radio Galaxies: Simulations and Emissions. We present a numerical study of the interactions between the elongated active galactic nuclei outflows representing an evolved, narrow-angle tail (NAT) radio galaxy and planar, transverse ICM shock fronts characteristic of those induced by galaxy clus... | [
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Untangling the Origin of Molecular Hydrogen in the Lunar Exosphere. In situ experiments from the Apollo missions confirmed the presence of a tenuous exosphere on the Moon comprised of atoms and light molecular species. Of the most prominent volatiles found in the exosphere, molecular hydrogen (H2) has drawn considerabl... | [
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Constraining the Stochastic Gravitational Wave from String Cosmology with Current and Future High-frequency Detectors. Pre-Big Bang models in string cosmology predict a relic background of gravitational wave radiation in the early universe. The spectrum of this background shows that the energy density rises rapidly wit... | [
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The Effect of Land Fraction and Host Star Spectral Energy Distribution on the Planetary Albedo of Terrestrial Worlds. The energy balance and climate of planets can be affected by the reflective properties of their land, ocean, and frozen surfaces. Here we investigate the effect of host star spectral energy distribution... | [
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Quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR Observations of the New X-Ray Clocked Burster 1RXS J180408.9-342058. We report the quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR observations showing spectral state transitions in the neutron star low-mass X-ray binary 1RXS J180408.9-342058 during its 2015 outburst. We pr... | [
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NuSTAR Observations of the Unidentified INTEGRAL Sources: Constraints on the Galactic Population of HMXBs. The NuSTAR Legacy program titled Unidentified INTEGRAL Sources targeted faint hard X-ray sources revealed by INTEGRAL in the Galactic plane in order to provide conclusive identification of their nature and insight... | [
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Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations. We study the orbital evolution and gravitational wave (GW) emission of supermassive black hole (SMBH) binaries formed in gas-free mergers of massive early-type galaxies using the hybrid tree-regularized N-body code KETJU. T... | [
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Model-independent Determination of Cosmic Curvature Based on the Padé Approximation. Given observations of the standard candles and cosmic chronometers, we apply Padé parameterization to the comoving distance and the Hubble parameter to find out how stringently the constraint is set to the curvature parameter by the da... | [
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The ALMA Spectroscopic Survey in the HUDF: Constraining Cumulative CO Emission at 1 ≲ z ≲ 4 with Power Spectrum Analysis of ASPECS LP Data from 84 to 115 GHz. We present a power spectrum analysis of the ALMA Spectroscopic Survey Large Program (ASPECS LP) data from 84 to 115 GHz. These data predominantly probe small-sca... | [
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The Sloan Digital Sky Survey Reverberation Mapping Project: Initial C IV Lag Results from Four Years of Data. We present reverberation-mapping (RM) lags and black hole mass measurements using the C IV λ1549 broad emission line from a sample of 348 quasars monitored as a part of the Sloan Digital Sky Survey RM Project. ... | [
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The Optically Thick Rotating Magnetic Wind from a Massive White Dwarf Merger Product. WD J005311 is a newly identified white dwarf (WD) in a mid-infrared nebula. The spectroscopic observation indicates the existence of a neon-enriched carbon/oxygen wind with a terminal velocity of {v}∞ ,{obs} ∼ 16,000 {km} {{{s}}}-1 an... | [
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Probing Coronal Magnetic Fields with Sungrazing Comets: H I Lyα from Pickup Ions. Observations of sungrazing comets can be used to probe the solar corona, to study the composition of the comets, and to investigate the plasma processes that govern the interaction between the coronal plasma and cometary gas. UVCS observa... | [
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Is the SNR HESS J1731-347 Colliding with Molecular Clouds?. The supernova remnant HESS J1731-347 is a young supernova remnant (SNR) that displays a nonthermal X-ray and TeV shell structure. A molecular cloud at a distance of ∼3.2 kpc is spatially coincident with the western part of the SNR, and it was likely hit by the... | [
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New Constraints on the Nuclear Equation of State from the Thermal Emission of Neutron Stars in Quiescent Low-mass X-Ray Binaries. This paper presents a new analysis of the thermal emission from the neutron star (NS) surface to constrain the dense matter equation of state. We employ an empirical parameterization of the ... | [
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The Gas-Star Formation Cycle in Nearby Star-forming Galaxies. I. Assessment of Multi-scale Variations. The processes regulating star formation in galaxies are thought to act across a hierarchy of spatial scales. To connect extragalactic star formation relations from global and kiloparsec-scale measurements to recent cl... | [
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Capability of Geomagnetic Storm Parameters to Identify Severe Space Weather. The paper investigates the capability of geomagnetic storm parameters in the disturbance storm-time (Dst), Kp, and AE indices to distinguish between severe space weather (SvSW) that causes the reported electric power outages and/or telecommuni... | [
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Detecting the 21 cm Signal from the Epoch of Reionization Using Drift Scans: Correlation of Time-ordered Visibilities. We present a formalism to extract the H I power spectrum from the epoch of reionization for drift scans using radio interferometers. Our main aim is to determine the coherence timescale of time-ordered... | [
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Mind the Gap: The Location of the Lower Edge of the Pair-instability Supernova Black Hole Mass Gap. Detections of gravitational waves are now starting to probe the mass distribution of stellar mass black holes (BHs). Robust predictions from stellar models are needed to interpret these. Theory predicts the existence of ... | [
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Modeling Collisional Excitation of [O I] Fine Structure Line Emission from PDRs. I. Homogeneous Clouds. Atomic oxygen (O0) plays a critical role in determining the structure of photon-dominated regions (PDRs), but reliable modeling of its emission has been hampered by the high optical depth of the 63 μm fine structure ... | [
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Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85. We present a physical characterization of MM J100026.36+021527.9 (a.k.a. “MAMBO-9”), a dusty star-forming galaxy (DSFG) at z = 5.850 ± 0.001. This is the highest-redshift unlensed DSFG (and fourth most distant overall) found to date and is... | [
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Fine-scale Explosive Energy Release at Sites of Prospective Magnetic Flux Cancellation in the Core of the Solar Active Region Observed by Hi-C 2.1, IRIS, and SDO. The second Hi-C flight (Hi-C 2.1) provided unprecedentedly high spatial and temporal resolution (∼250 km, 4.4 s) coronal EUV images of Fe IX/X emission at 17... | [
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Nonstationary Fast-driven, Self-organized Criticality in Solar Flares. The original concept of self-organized criticality, applied to solar flare statistics, assumed a slow-driven and stationary flaring rate, which implies timescale separation (between flare durations and interflare waiting times). The concept reproduc... | [
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Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations. We present a statistical analysis of the flybys of dark matter halos compared to mergers, using cosmological N-body simulations. We mainly focus on gravitationally interacting target halos with mass o... | [
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Line Expansion Opacity in Relativistically Expanding Media. Spectral lines of heavy atomic elements in the ejecta of supernovae and neutron star mergers can have important contribution to the opacity of the ejecta matter even when the abundance of the elements is very small. Under favorable conditions, the line expansi... | [
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Perpendicular Ion Heating by Cyclotron Resonant Dissipation of Turbulently Generated Kinetic Alfvén Waves in the Solar Wind. Solar wind ions are observed to be heated in the directions perpendicular to the large-scale magnetic field, with preferential heating given to heavy ions. In the solar corona, this heating may b... | [
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Magnetic Helicity Budget of Solar Active Regions Prolific of Eruptive and Confined Flares. We compare the coronal magnetic energy and helicity of two solar active regions (ARs), prolific in major eruptive (AR 11158) and confined (AR 12192) flaring, and analyze the potential of deduced proxies to forecast upcoming flare... | [
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Kinematics: A Clean Diagnostic for Separating Supernova Remnants from H II Regions in Nearby Galaxies. Many more supernova remnants (SNRs) are now known in external galaxies than in the Milky Way. Most of these SNRs have been identified using narrowband imaging, separating SNRs from H II regions on the basis of [S II]:... | [
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Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae. Some binary systems composed of a white dwarf (WD) and a hot subdwarf (sdB) helium star will make contact within the helium burning lifetime of the sdB star. The accreted helium on the WD inevitably undergoes a thermonucl... | [
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Laboratory Formation and Photochemistry of Fullerene/Anthracene Cluster Cations. Besides buckminsterfullerene (C60), other fullerenes and their derivatives may also reside in space. In this work, we study the formation and photodissociation processes of astronomically relevant fullerene/anthracene (C14H10) cluster cati... | [
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Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions. We report on observations of the two newly identified reconnection geometries involving erupting flux ropes. In 3D, a flux rope can reconnect either with a surrounding coronal arcade (recen... | [
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Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection. We calculate the evolution of massive stars, which undergo pulsational pair-instability (PPI) when the O-rich core is formed. The evolution from the main sequence through the onset of PPI is calculated for stars with initi... | [
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A Data-driven Model of Nucleosynthesis with Chemical Tagging in a Lower-dimensional Latent Space. Chemical tagging seeks to identify unique star formation sites from present-day stellar abundances. Previous techniques have treated each abundance dimension as being statistically independent, despite theoretical expectat... | [
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ALMA Reveals a Gas-rich, Maximum Starburst in the Hyperluminous, Dust-obscured Quasar W0533-3401 at z ∼ 2.9. We present ALMA observations and multiwavelength spectral energy distribution analysis in a Wide-field Infrared Survey Explorer-selected, hyperluminous dust-obscured quasar W0533-3401 at z = 2.9. We derive the p... | [
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Supernova 2014C: Ongoing Interaction with Extended Circumstellar Material with Silicate Dust. Supernova (SN) 2014C is unique: a seemingly typical hydrogen-poor SN that started to interact with a dense, hydrogen-rich circumstellar medium (CSM) ∼100 days post-explosion. The delayed interaction suggests a detached CSM she... | [
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Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1. We present a detailed high-resolution weak-lensing study of SPT-CL J2106-5844 at z = 1.132, claimed to be the most massive system discovered at z > 1 in the South Pole Telescope Sunyaev-Zel’dovich survey. Based on the deep imaging... | [
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Modeling Energetic Particle Acceleration and Transport in a Solar Wind Region with Contracting and Reconnecting Small-scale Flux Ropes at Earth Orbit. New analytical steady-state and time-dependent solutions for the acceleration of energetic particles by contracting and reconnecting small-scale flux ropes (SMFRs) in th... | [
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Nature and Origins of Rich Complexes of C IV Associated Absorption Lines. Rich complexes of associated absorption lines (AALs) in quasar spectra provide unique information about gaseous infall, outflows, and feedback processes in quasar environments. We study five quasars at redshifts z ~ 3.1-4.4 with AAL complexes con... | [
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The Interaction between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30. G23.33-0.30 is a 600 M ⊙ infrared dark molecular filament that exhibits large NH3 velocity dispersions (σ ∼ 8 km s-1) and bright, narrow NH3(3, 3) line emission. We have probed G23.33-0.30 at the < 0.1 pc scale and... | [
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Mapping Metallicity Variations across Nearby Galaxy Disks. The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution remains poorly sampled. We have determined the gas phase oxygen abundances for 7138 H II regions across the... | [
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A Hybrid Approach Toward Simulating Reionization: Coupling Ray Tracing with Excursion Sets. This paper introduces a new method of generating 21 cm maps that is based on ideas from ray tracing and excursion sets. In this method, photons generated in each grid cell are computed using the excursion set ideas while their p... | [
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Stellar Pulsation and the Production of Dust and Molecules in Galactic Carbon Stars. New infrared spectra of 33 Galactic carbon stars from FORCAST on SOFIA reveal strong connections between stellar pulsations and the dust and molecular chemistry in their circumstellar shells. A sharp boundary in overall dust content, w... | [
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Validation of the Alfvén Wave Solar Atmosphere Model (AWSoM) with Observations from the Low Corona to 1 au. We perform a validation study of the latest version of the Alfvén Wave Solar atmosphere Model (AWSoM) within the Space Weather Modeling Framework. To do so, we compare the simulation results of the model with a c... | [
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Stellar Chromospheric Activity and Age Relation from Open Clusters in the LAMOST Survey. We identify member stars of more than 90 open clusters in the LAMOST survey. With the method of Fang et al., the chromospheric activity (CA) indices, {log}{R}CaK}{\prime } for 1091 member stars in 82 open clusters and {log}{R}{{H}α... | [
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Predicting Lyα Emission from Galaxies via Empirical Markers of Production and Escape in the KBSS. Lyα emission is widely used to detect and confirm high-redshift galaxies and characterize the evolution of the intergalactic medium (IGM). However, many galaxies do not display Lyα emission in typical spectroscopic observa... | [
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"http://astrothesaurus.org/uat/1379",
"http://astrothesaurus.org/uat/1383",
"http://astrothesaurus.org/uat/1558"
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The Nearby, Young, χ <SUP>1</SUP> Fornacis Cluster: Membership, Age, and an Extraordinary Ensemble of Dusty Debris Disks. Only four star clusters are known within ∼100 pc of Earth. Of these, the χ 1 For cluster has barely been studied. We use the Gaia DR2 catalog and other published data to establish the cluster member... | [
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The Nature of Ionized Gas in the Milky Way Galactic Fountain. We address the spatial scale, ionization structure, mass, and metal content of gas at the Milky Way disk-halo interface detected as absorption in the foreground of seven closely spaced, high-latitude halo blue horizontal branch stars with heights z = 3-14 kp... | [
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"http://astrothesaurus.org/uat/699",
"http://astrothesaurus.org/uat/1879",
"http://astrothesaurus.org/uat/810"
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A Trio of Massive Black Holes Caught in the Act of Merging. We report the discovery of SDSS J0849+1114 as the first known triple Type 2 Seyfert nucleus. It represents three active black holes that are identified from new spatially resolved optical slit spectroscopy using the Dual Imaging Spectrograph on the 3.5 m teles... | [
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Chemical Abundances along the 1G Sequence of the Chromosome Maps: The Globular Cluster NGC 3201. The Hubble Space Telescope (HST) UV Legacy Survey of Galactic Globular Clusters (GCs) has investigated multiple stellar populations by means of the “chromosome map” (ChM) diagnostic tool that maximizes the separation betwee... | [
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The Distribution of Ultra-diffuse and Ultra-compact Galaxies in the Frontier Fields. Large low-surface-brightness galaxies have recently been found to be abundant in nearby galaxy clusters. In this paper, we investigate these ultra-diffuse galaxies (UDGs) in the six Hubble Frontier Fields galaxy clusters: A2744, MACS J... | [
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A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS. We present a new three-dimensional map of dust reddening, based on Gaia parallaxes and stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a decl. of -30°, out to a distance of a few kiloparsecs. This new map contains three major improve... | [
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"http://astrothesaurus.org/uat/621",
"http://astrothesaurus.org/uat/837",
"http://astrothesaurus.org/uat/853"
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The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles. Dark-matter-only simulations predict that dark matter halos have steep, cuspy inner density profiles, while observations of dwarf galaxies find a range of inner slopes that are often much shallower. There is debate whether this dis... | [
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Expansion of Solar Coronal Hot Electrons in an Inhomogeneous Magnetic Field: 1D PIC Simulation. The expansion of hot electrons in flaring magnetic loops is crucial to understanding the dynamics of solar flares. In this paper we investigate, for the first time, the transport of hot electrons in a magnetic mirror field b... | [
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Multivariate Analysis of BATSE Gamma-Ray Burst Properties Using Skewed Distributions. The number of classes of gamma-ray bursts (GRBs), besides the well-established short and long ones, remains a debatable issue. It was already shown, however, that when invoking skewed distributions, the {log}{T}90 and {log}{T}90-{log}... | [
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Accelerated Expansion of the Universe in the Model with Nonuniform Pressure. We present the particular case of the Stephani solution for shear-free perfect fluid with uniform energy density and nonuniform pressure. Such models appeared as possible alternative to the consideration of the exotic forms of matter like dark... | [
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Energy Origination and Triggering Mechanism of a Series of Homologous Confined Flares. Using the Hα data from the New Vacuum Solar Telescope at the Fuxian Solar Observatory together with multiwavelength images and magnetograms obtained by the Solar Dynamics Observatory, we study the detailed process of three homologous... | [
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Spallation-altered Accreted Compositions for X-Ray Bursts: Impact on Ignition Conditions and Burst Ashes. Model predictions of X-ray burst ashes and light curves depend on the composition of the material accreted from the companion star, in particular the abundance of CNO elements. It has previously been pointed out th... | [
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Spectral and Timing Properties of the Galactic X-Ray Transient Swift J1658.2-4242 Using Astrosat Observations. We present the X-ray timing and spectral analysis of the new Galactic X-ray transient Swift J1658.2-4242 observed with the Large Area X-ray Proportional Counter and Soft X-ray Telescope instruments on board As... | [
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Propagation of Scatter-free Solar Energetic Electrons in a Meandering Interplanetary Magnetic Field. We investigate energetic electron transport in a meandering interplanetary magnetic field under the scatter-free regime. The meandering magnetic field is adopted from the Giacalone model in which a single parameter V rm... | [
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Exploring Plasma Heating in the Current Sheet Region in a Three-dimensional Coronal Mass Ejection Simulation. We simulate a coronal mass ejection using a three-dimensional magnetohydrodynamic code that includes coronal heating, thermal conduction, and radiative cooling in the energy equation. The magnetic flux distribu... | [
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Type Ia Supernovae Are Excellent Standard Candles in the Near-infrared. We analyze a set of 89 type Ia supernovae (SNe Ia) that have both optical and near-infrared (NIR) photometry to derive distances and construct low-redshift (z ≤ 0.04) Hubble diagrams. We construct mean light curve (LC) templates using a hierarchica... | [
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Massive-star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores. Similar to their low-mass counterparts, massive stars likely form via the collapse of prestellar molecular cores. Recent observations suggest that most massive cores are subvirial (i.e., not supported by turbulence) and therefo... | [
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Eclipsing Binaries in the Open Cluster Ruprecht 147. II. Epic 219568666. We report our spectroscopic monitoring of the detached, grazing, and slightly eccentric 12 day double-lined eclipsing binary EPIC 219568666 in the old nearby open cluster Ruprecht 147. This is the second eclipsing system to be analyzed in this clu... | [
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Influence of Density Dependence of Symmetry Energy in Hot and Dense Matter for Supernova Simulations. We study the influence of density-dependent symmetry energy at high densities in simulations of core-collapse supernovae, black hole formation, and proto-neutron star cooling by extending the relativistic mean field (R... | [
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Mapping Spatial Variations of H I Turbulent Properties in the Small and Large Magellanic Cloud. We developed methods for mapping spatial variations of the spatial power spectrum (SPS) and structure function slopes, with the goal of connecting the statistical properties of neutral hydrogen (H I) with the turbulent drive... | [
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Star Formation Histories of the LEGUS Dwarf Galaxies. III. The Nonbursty Nature of 23 Star-forming Dwarf Galaxies. We derive the recent star formation histories (SFHs) of 23 active dwarf galaxies using Hubble Space Telescope observations from the Legacy Extragalactic UV Survey. We apply a color-magnitude diagram (CMD) ... | [
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Unbiased Differential Size Evolution and the Inside-out Growth of Galaxies in the Deep CANDELS GOODS Fields at 1 ≤ z ≤ 7. We present a size analysis of a sample of ∼49,000 galaxies from the Cosmic Assembly Near-infrared Deep Extragalactic Survey GOODS North and South fields, using redshift-independent relative surface-... | [
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Metallicity Structure in the Milky Way Disk Revealed by Galactic H II Regions. The metallicity structure of the Milky Way disk stems from the chemodynamical evolutionary history of the Galaxy. We use the National Radio Astronomy Observatory Karl G. Jansky Very Large Array to observe ∼8-10 GHz hydrogen radio recombinati... | [
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Spectroscopy of the Young Stellar Association Price-Whelan 1: Origin in the Magellanic Leading Arm and Constraints on the Milky Way Hot Halo. We report spectroscopic measurements of stars in the recently discovered young stellar association Price-Whelan 1 (PW 1), which was found in the vicinity of the Leading Arm (LA) ... | [
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Compressible and Incompressible Magnetic Turbulence Observed in the Very Local Interstellar Medium by Voyager 1. Voyager 1 observed Kolmogorov-like (k -5/3) compressible turbulence just upwind of the heliopause. Subsequent measurements by Voyager 1 further from the heliopause revealed that the observed fluctuations wer... | [
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Turbulent Heating in Solar Wind Thermodynamics. This paper considers the concept of wave-particle thermodynamic equilibrium in order to improve our understanding of the role of turbulent heating in the solar wind proton plasma. The thermodynamic equilibrium in plasmas requires the energy of a plasmon—the quantum of pla... | [
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Observational Analysis on the Early Evolution of a CME Flux Rope: Preflare Reconnection and Flux Rope’s Footpoint Drift. We study the early evolution of a hot-channel-like magnetic flux rope (MFR) toward eruption. Combining with imaging observation and magnetic field extrapolation, we find that the hot channel possibly... | [
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Narrow-absorption Line Complex. IV. Line-driven Radiative Outflows in Broad-absorption Line Quasars. It has been reported that some broad-absorption lines (BALs) in quasar spectra can be decomposed into multiple narrow-absorption lines (NALs), which we define as “Type N BALs.” In this paper, using the spectra of 2005 B... | [
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High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth. As computational resolution of modern cosmological simulations come closer to resolving individual star-forming clumps in a galaxy, the need for “resolution-appropriate” physics for a galaxy-... | [
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