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Response of Martian Tail Lobes to Heliospheric Current Sheet: Tianwen-1 and MAVEN Joint Observations. Martian magnetotail lobes, mainly formed by the draped interplanetary magnetic field extending downstream in the tailward direction, are largely controlled by the solar wind and respond sensitively to variations in ups... | [
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The Magnitude of the Dark Ages 21 cm Signal in the Context of Existing Early and Late Time Constraints on ΛCDM. The dark ages 21 cm signal is a promising probe of the currently unobserved infant Universe between the formation of the cosmic microwave background around z ≍ 1100 and the first galaxies around z ≍ 30. A det... | [
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Intertwined Birth and Death: A Herbig─Haro Outflow Resolves the Distance to Vela Junior. The distance to the Vela Junior supernova remnant (RX J0852.0─4622 or G266.2─1.2) has long remained uncertain, limiting our understanding of its physical properties. Using Very Large Telescope/Multi Unit Spectroscopic Explorer inte... | [
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Revised Active Galactic Nuclei Spectral Model Reveals a More Significant Role in Cosmic Reionization. Reionization marks one of the most important phase transitions in the history of the Universe, during which neutral baryonic matter was transformed into ionized plasma. While star-forming galaxies are widely regarded a... | [
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A Cool Earth-sized Planet Candidate Transiting a Tenth Magnitude K-dwarf From K2. The transit method is currently one of our best means for the detection of potentially habitable "Earth-like" exoplanets. In principle, given sufficiently high photometric precision, cool Earth-sized exoplanets orbiting Sun-like stars cou... | [
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Hour-scale Variations of Water Molecules in the Lunar Soil Revealed by Chang'e-6 In Situ Observations. The speciation, inventory, and dynamic changes of water (OH/H2O) on the lunar surface remain poorly constrained. The Chang'e-6 (CE-6) mission conducted in situ spectroscopic measurements of lunar water over time inter... | [
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Extreme Winds on the Emerging Dayside of an Ultrahot Jupiter. High-resolution spectroscopy provides a unique opportunity to directly probe atmospheric dynamics by resolving Doppler shifts of planetary signals as a function of orbital phase. Using the optical spectrometer the Keck Planet Finder, we carry out a pilot stu... | [
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Double Hot Jupiter Formation through Mirrored ZLK Migration in Binary Star Systems: The Case of WASP-94. To date, only a handful of binary star systems are known with at least one confirmed planet orbiting each star. Such systems, however, offer a unique perspective on the stochasticity intrinsic to planet formation an... | [
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Characterizing Alfvénicity and Proton Temperature Distributions in Interplanetary Coronal Mass Ejection Magnetic Clouds. We investigated a comprehensive sample of 474 interplanetary coronal mass ejection (ICME) events observed by the Wind spacecraft to examine the Alfvénic characteristics within their magnetic cloud re... | [
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Dark-matter-deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics. High-velocity collisions between gas-rich ultradiffuse galaxies present a promising formation channel for dark-matter-deficient galaxies (DMDGs). Using hydrodynamical simulations, we show that the progenitors' baryon... | [
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CECILIA: Gas-phase Physical Conditions and Multielement Chemistry at Cosmic Noon. Galaxies at Cosmic Noon (z ∼ 2─3) are characterized by rapid star formation that will lead to significant metal enrichment in the interstellar medium (ISM). While much observational evidence suggests that these galaxies are chemically dis... | [
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On the Ultralong Gamma-Ray Transient GRB 250702B/EP 250702a. GRB 250702B/EP 250702a is an interesting long-duration gamma-ray transient whose nature is in debate. To obtain a full picture in the gamma-ray band, we implement a comprehensive targeted search of burst emission in a wide window of 30 days jointly with Insig... | [
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Using Gravity as an Age Indicator for Young Stars. The age of a young star is difficult to measure and yet is a fundamental property that is essential for understanding stellar evolution. Accurate age indicators across the early phases of low-mass stars are scarce and often rely on properties of the circumstellar envir... | [
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exoALMA. XIX. Confirmation of Non-thermal Line Broadening in the DM Tau Protoplanetary Disk. Turbulence is expected to transport angular momentum and drive mass accretion in protoplanetary disks. One way to directly measure turbulent motion in disks is through molecular line broadening. DM Tau is one of only a few disk... | [
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IK Pegasi and the Double-merger Path to Type Ia Supernovae. Recent Gaia astrometry has revealed thousands of main-sequence + white dwarf (MS+WD) binaries at separations of ∼0.1─10 au, including a subset hosting unusually massive (≳0.8M⊙) WDs. We argue that s-process enrichment in the nondegenerate companion provides a ... | [
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Composition and Space-weathering Characteristics of the Tianwen-2 Mission's First Target: Near-Earth Asteroid (469219) Kamo'oalewa. The near-Earth asteroid Kamo'oalewa, a quasi-satellite of the Earth and the first target for sample return by China's Tianwen-2 mission, exhibits distinctive spectral characteristics. This... | [
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Extreme-ultraviolet Synthesis of Nanojet-like Ejections due to Coalescing Flux Ropes. Detection and characterization of small-scale energetic events such as nanoflares and nanojets remain challenging owing to their short lifetimes, small spatial extent, and relatively low energy release, despite their potential role in... | [
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A τ─DM Relation for Fast Radio Burst Hosts?. It has been proposed that measurements of scattering times (τ) from fast radio bursts (FRBs) may be used to infer the FRB host dispersion measure (DM) and its redshift. This approach relies on the existence of a correlation between τ and DM within FRB hosts such as that obse... | [
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Machine Learning versus Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation. Traditional spectral energy distribution (SED)─fitting methods for stellar mass estimation face persistent challenges including systematic biases and computational constraints. We present a contr... | [
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The Proper Motion of Draco II with HST Using Multiple Reference Frames and Methodologies. We present proper motion (PM) measurements for Draco II, an ultrafaint dwarf satellite of the Milky Way. These PMs are measured using two epochs of Hubble Space Telescope (HST)/Advanced Camera for Surveys imaging separated by a 7 ... | [
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Insights from Analytical Theory of Eccentric Circumbinary Disks. Eccentric cavities in circumbinary disks precess on timescales much longer than the binary orbital period. These long-lived steady states can be understood as trapped modes in an effective potential primarily determined by the binary quadrupole and the in... | [
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The Nature of Nitrogen-enhanced High-redshift Galaxies. Recent JWST observations have revealed a population of high-redshift galaxies (z ≳ 5) exhibiting unexpectedly bright ultraviolet (UV) nitrogen emission lines. The strong N III] and N IV] features imply nitrogen-to-oxygen abundance ratios (N/O) as high as −0.8≲log... | [
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Time-dependent Modeling of the Subhour Spectral Evolution during the 2013 Outburst of Mrk 421. In 2013 April, the TeV blazar Markarian 421 underwent one of its most powerful emission outbursts recorded to date. An extensive multi-instrument campaign featuring MAGIC, VERITAS, and NuSTAR provided comprehensive very high-... | [
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Probing the Molecular Hearts of Extreme Bipolar Planetary Nebulae with ALMA. We present results from a program of Atacama Large Millimeter Array (ALMA) 1.3 mm (Band 6) molecular line mapping of a sample of nearby, bipolar/pinched-waist, molecule-rich planetary nebulae (PNs; NGC 6302, Hubble 5, NGC 2440, NGC 6445, NGC 2... | [
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Strategy for Identifying Vera C. Rubin Observatory Kilonova Candidates for Targeted Gravitational-wave Searches. Since the observation of the binary neutron star merger GW170817 and the associated kilonova AT2017gfo, the next joint gravitational-wave/optical kilonova has been highly anticipated. Overlapping observation... | [
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Turbulent Modes in Slow, Alfvénic Slow, and Fast Solar Wind at 1 au. The characterization of solar wind fluctuations provides insight into magnetofluid turbulence. The slow solar wind with high Alfvénicity, the Alfvénic slow solar wind (ASSW), possesses a similar bulk speed as the slow wind, but with fluctuations large... | [
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"http://astrothesaurus.org/uat/1534",
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Double Stars, Double Disks: Discovering the Young Companion of Herbig Be Star MWC 340. We present the discovery of a young, close-in companion to the early B-type Herbig Be star MWC 340 (V1685 Cyg), a rare system known to host a protoplanetary disk. Herbig Be stars often show complex circumstellar environments shaped b... | [
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Kink Oscillations of Curved Arcade Loops with a Magnetic Shear. We considered the kink oscillations of coronal magnetic loops, which form a coronal loop arcade with a magnetic shear. In this structure, the magnetic field consists of helical lines. A semicircular magnetic slab model was used, and the corresponding dispe... | [
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Energetically Dominant Sunward-propagating Alfvén Waves near 1 au and Their Relation to Large-scale Magnetic Switchbacks. In this paper, we investigate the population of energetically dominant sunward-propagating Alfvén waves (SAWs) using more than 20 yr of data provided by the Wind spacecraft near 1 au. We refer to SA... | [
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Shock Wave Precursors in M33 Supernova Remnants. We present high-resolution profiles of the Hα, [N II], and [O III] lines of supernova remnants (SNRs) in M33. The 8 km s−1 resolution allows us to separate emission from the photoionized shock precursors from the emission from shocked gas. We find that there is considera... | [
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Machine Learning Estimation of Energy Fractions in Magnetohydrodynamic Turbulence Modes. Magnetohydrodynamic (MHD) turbulence plays a central role in many astrophysical processes in the interstellar medium (ISM), including star formation and cosmic-ray transport and acceleration. MHD turbulence can be decomposed into t... | [
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Investigating the Anisotropy of Dispersion Measure Contribution from the Galactic Halo by Using Fast Radio Bursts. We propose a data-driven approach to reconstruct the all-sky distribution of the dispersion measure contribution from the Galactic halo (DMhalo) through a spherical harmonic expansion, enabling an investig... | [
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Observation of the Forbush Decrease on 2024 May 10, Using the ALPAQUITA Air-shower Array at the 70─1000 GV Rigidity Range. The Andes Large area PArticle detector for Cosmic ray physics and Astronomy is a new air-shower array experiment under construction in the Bolivian Andes, and its prototype ALPAQUITA surface array ... | [
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Causal Relationship between Current Sheet Flapping, Electron-only Reconnection, and Ion-coupled Reconnection. Magnetic reconnection is a fundamental physical process operating throughout the Universe, yet its onset in planetary magnetotails remains elusive. Current-sheet flapping is a common dynamic phenomenon in plane... | [
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Impact of Propagation Effects on the Spectro-temporal Properties of Fast Radio Bursts. We present a mathematical analysis of propagation-induced distortions in the spectro-temporal properties of fast radio bursts (FRBs). Within the triggered relativistic dynamical model, we derive a centroid-based formulation of the su... | [
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MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites. Giant low-surface-brightness galaxies (gLSBGs) are rare objects with disk radii up to 160 kpc and dynamical masses of up to the order of 1012 M⊙. Their very existence challenges currently accepted theories of galaxy formation and evolution... | [
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A Quenched and Relatively Isolated Dwarf Galaxy in the Local Volume. An increasing number of discoveries of isolated and quenched dwarf galaxies are challenging the idea that the present-day local environment of low-mass systems is the main determinant of their quenching. We present new Hubble Space Telescope (HST) dat... | [
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Surface Interactions in Photon Monte Carlo Simulations. We implement a comprehensive simulation of photon surface interactions using a Monte Carlo approach. This is effective in simulating the interaction of light with telescope mirrors and lenses. We use a full electromagnetic solution to simulate the wavelength and a... | [
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Super-Eddington Accretion onto Black Holes and Its Application to Fallback Accretion. We study the problem of steady-state spherical accretion onto a black hole, in which the internal energy of the flow is governed by radiation and photon diffusion dominates the energy flux at large radii. In the freefall limit, the fl... | [
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Numerical Simulations of the Circularized Accretion Flow in Population III Star Tidal Disruption Events. I. The Accretion Flow and the Wind. Tidal disruption events (TDEs) have recently been proposed as potential probes for Population III (Pop III) stars. However, the properties of the accretion flow and the wind from ... | [
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Evidence for the Transition from Thermal to Nonthermal Emission in the Prompt Emission of GRB 161117A. GRB 161117A is a long-duration gamma-ray burst with three main overlapping peaks. By analyzing the time-resolved spectra of its data observed with the Gamma-Ray Burst Monitor on board the Fermi mission, we find that t... | [
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A Solution to the Tension of Burning on Neutron Stars and Nuclear Physics. When neutron stars accrete matter from a companion star, this matter forms a disk around them and eventually falls on their surface. Here, the fuel can ignite into bright flashes called Type I bursts. Theoretical calculations based on state-of-t... | [
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Unveiling the Ionized and Neutral ISM at z > 10: The Origin of [O III] /[C II] Ratios from a Subparsec Resolution Radiative Transfer Simulation. Recent multiwavelength observations by JWST and the Atacama Large Millimeter/submillimeter Array (ALMA) are unveiling both ionized and neutral interstellar medium (ISM) com... | [
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Infrared Spectral Energy Distribution Modeling of Velocity Excess in Maser Sources: Identifying Incipient Water Fountain Candidates. We investigated whether "velocity excess" in circumstellar maser lines can diagnose the earliest evolutionary phases of water fountains (WFs). Here, we define "velocity excess" as maser e... | [
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Evolution of a Long-lived Deep-seated Main-sequence Magnetic Field during White Dwarf Cooling. We study the evolution of white dwarf (WD) magnetic fields that originate from convective-core dynamos during the main sequence. Using stellar evolution and WD cooling models combined with magnetic field diffusion calculation... | [
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Predicting Dust Temperature from Molecular Line Data Using Machine Learning. We have conducted experiments with machine learning techniques to construct dust temperature maps from the CO isotopolog molecular line data in the Orion A molecular cloud. In classical astrophysical methodology, multiband continuum data are r... | [
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On the Origin of Intracluster Light Based on the High-resolution Simulation, NEWCLUSTER. Intracluster light (ICL) is a key component of galaxy clusters, with the potential to trace their dynamical assembly histories and the underlying dark matter distribution. Despite these prospects, its faint nature makes a consensus... | [
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Absolute Properties of Two Double-lined Algol-type Binaries with Cyclic Period Changes. The formation, evolution, and stability of multiple star systems are still open questions in the field of astrophysics. Algol-type binaries are important for obtaining precise physical parameters, investigating the reversal of the m... | [
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Tides in Massive Binaries: Numerical Solutions and Semianalytical Comparisons. We present a systematic comparison between the tidal secular evolution timescales predicted by the direct numerical method and those given by the commonly used semianalytic prescriptions implemented in 1D hydrostatic binary evolution codes. ... | [
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A Correlation between the Final Separation and Mass Ratio from Common-envelope Simulations. Analytical models for common-envelope evolution (CEE), particularly the energy formalism, are used in binary population synthesis to predict post-CEE configurations. This formalism is based on an efficiency parameter α, which re... | [
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A Closer Look at the Dynamical State of the High-redshift Galaxy Cluster SPT-CL J2215-3537. We present a comprehensive reanalysis of the dynamical state of the high-redshift galaxy cluster SPT-CL J2215-3537 (z = 1.16), using the full set of available Chandra observations to characterize the thermodynamic and morphologi... | [
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Accretion Geometry of the New Galactic Black Hole Candidate AT2019wey in the Hard State. We perform broadband spectral and timing studies of the Galactic low-mass black hole candidate AT2019wey using quasi-simultaneous NICER, Swift, and NuSTAR observations obtained in 2022. The long-term MAXI light curve, along with th... | [
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Time-integrated Southern-sky Neutrino Source Searches with 10 yr of IceCube Starting-track Events at Energies Down to 1 TeV. In the IceCube Neutrino Observatory, a signal of astrophysical neutrinos is obscured by backgrounds from atmospheric neutrinos and muons produced in cosmic-ray interactions. IceCube event selecti... | [
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No Evidence for Second-scale Periodicity in FRB 20201124A from 2021 April to June FAST Observations. Fast radio bursts (FRBs) are bright and short radio flashes of cosmological origin. Although a great number of FRBs have been detected in the last two decades, their progenitors and the physical processes that create th... | [
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The Astrophysical Birth Environment of the Solar System Inferred from Cometary Noble Gases. The stellar sources that contributed to the chemical and isotopic composition of the solar system, their mixing in the Galactic environment, and the evolution and longevity of the molecular cloud from which our solar system form... | [
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JWST/NIRSpec Detects Warm CO Emission in the Terrestrial-planet Zone of HD 131488. We have obtained a high-resolution, JWST NIRSpec 2.87─5.14 μm spectrum of the debris disk around HD 131488. We discover CO fundamental emission indicating the presence of warm fluorescent gas within ∼10 au of the star. The large discrepa... | [
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Globular Cluster Systems in Dwarf Galaxies: Catalogs and Comparisons. The connection between a galaxy's total globular cluster system (GCS) mass and its halo mass has been studied for decades and it has been found that galaxies at nearly all observed masses adhere to a linear scaling relation between these properties. ... | [
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ALMA Lensing Cluster Survey: Molecular Gas Properties of Line-emitting Galaxies from a Blind Survey. We present results of a blind search for line-emitting galaxies using Atacama Large Millimeter/submillimeter Array (ALMA) Lensing Cluster Survey data. We detected seven line emitters, one of which is [C II] at z = 6.071... | [
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Taming the Plunge: A Circularization Trap of Supermassive Black Hole Binaries. We investigate the orbital eccentricity evolution of supermassive black hole binaries (SMBHBs; 104─107 M⊙) within galactic environments. Merger timescales depend on eccentricity when gravitational-wave (GW) emission dominates. We analyze the... | [
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Unified g- and r-mode Analysis of Accreting White Dwarf Stars. Dwarf novae are a subset of cataclysmic variables that accrete material intermittently in short-duration outbursts with sometimes long quiescent intervals in between. During the quiescent state, the white dwarf (WD) photosphere may be observable. Some of th... | [
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Particle Transport from First Principles in the Early Heliosphere: κ<SUP>1</SUP> Ceti as a Case Study for the Young Sun. Several studies of Galactic cosmic-ray (GCR) modulation within the astrospheres of stars deemed to be proxies for the young Sun have concluded that the intensities of these particles would, at early ... | [
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Origins of Mercury's Big Heart of Iron: Exploring Pathways to Form High Core Mass Fraction Planets via N-body Simulations. Mercury's core mass fraction (CMF) is 0.7, more than double that of the other rocky planets in the solar system, which have CMFs of 0.3 or lower. The origin of Mercury's large, iron-rich core remai... | [
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Chemodynamics of Boötes I with S<SUP>5</SUP>: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints. We combine new spectroscopic observations of the ultrafaint dwarf (UFD) galaxy Boötes I (Boo I) from the Southern Stellar Stream Spectroscopic Survey (S5) with ∼15 yr of archival sp... | [
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Tracking the Assembly of Supermassive Black Holes: A Comparison of Diverse Models across Cosmic Time. Galaxies grow alongside central supermassive black holes (SMBHs) through fueling and feedback. However, the origins of this coevolution remain unclear and vary across modeling frameworks. Using semianalytic models (SAM... | [
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The Strongly Lensed Hα-emitting Galaxy Population at 3.8 < z < 6.6. Hα luminosity traces the ionizing-photon output of short-lived, massive stars and is therefore a key diagnostic of star formation in high-redshift galaxies. Recent JWST observations have delivered updated Hα luminosity functions (LFs) of Hα-emitt... | [
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Betelgeuse: Detection of the Expanding Wake of the Companion Star. Recent analyses conclude that Betelgeuse, a red supergiant star (HD 39801), likely has a companion object with a period of ∼2000 days orbiting at only 2.3 R⋆, deep in the chromosphere of the supergiant. A probable detection of such a companion, named Si... | [
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Tracking the Evolution of Plasma Instabilities from the Prominence─Corona Transition Region into Interplanetary Space with Total Solar Eclipse and PSP/WISPR White Light Images. High-resolution total solar eclipse (TSE) white light (WL) images are the only observations at present to capture coronal structures over an un... | [
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Diffusion-free Dynamics in Rotating Spherical Shell Convection Driven by Internal Heating and Cooling. The bulk properties of convection in stellar and giant planet interiors are often assumed to be independent of the molecular diffusivities, which are very small. By contrast, simulations of this process in rotating sp... | [
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ALMA Band 7 Observations of Water Lines in the Protoplanetary Disk of V883 Ori. The FU Orionis star V883 Ori provides a unique opportunity to probe the water snowline in a protoplanetary disk. During an accretion burst, the enhanced stellar luminosity heats the disk, sublimating ices and bringing volatile species into ... | [
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Spectroscopic Follow-up of Gaia Alerted Young Stellar Object Variables: The Large Binocular Telescope View. We analyzed optical/near-IR Large Binocular Telescope spectra of 16 sources alerted by Gaia between 2021 and 2024 due to significant photometric variability. Half of the spectra were taken during quiescence and t... | [
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Asteroseismology for Probing the Interior Structure and Orbital Stability of Extremely Low Mass Ratio Contact Binaries. Theoretical investigations predict a minimum mass ratio of about 0.085─0.095 for contact binaries. If the mass ratio is below the critical value, a tidal instability occurs, forcing the stars to merge... | [
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FEASTS Compared with Simulations: Abnormally Irregular and Extended H I Morphologies at a Column Density of 10<SUP>18</SUP> cm<SUP>−2</SUP> in TNG50 and Auriga. With new atomic-hydrogen (H I) observations of FAST Extended Atlas of Selected Targets Survey (FEASTS), we present the first statistical comparison of H I morp... | [
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Ignition of Weak Interactions and r-process Outflows in Supercollapsar Accretion Disks. The collapse of rotating massive (∼10M⊙) stars resulting in hyperaccreting black holes (BHs; "collapsars") is a leading model for the central engines of long-duration gamma-ray bursts (GRBs) and a promising source of rapid neutron-c... | [
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A Mysterious Feature in the NICER Spectrum of 4U 1820-30: A Gravitationally Redshifted Absorption Line?. A mysterious absorption feature at approximately 3.8 keV has been identified in the Neutron star Interior Composition Explorer (NICER) spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this featu... | [
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Death by Impact: Evidence for Merger-driven Quenching in a Collisional Ring Galaxy at Cosmic Noon. The role of interactions and mergers in the rapid quenching of massive galaxies in the early Universe remains uncertain, largely due to the difficulty of directly linking mergers to quenching. Collisional ring galaxies pr... | [
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Broad-line Regions behind Haze: The Intrinsic Shape of the Brγ Line and Its Origin in a Type 1 Seyfert Galaxy. The broad-line region (BLR) of active galactic nuclei is an essential component, yet its small size keeps its origin, structure, and kinematics uncertain. Infrared interferometry with VLTI/GRAVITY is now resol... | [
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Particle Acceleration and Depolarization in the Protostellar Jet Knots HH 80 and HH 81. Linearly polarized emission is a powerful tracer of magnetic field geometry and particle acceleration in protostellar jets. We present a polarimetric study of the Herbig─Haro (HH) objects HH 80 and HH 81, where nonthermal emission h... | [
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Hierarchical Test of Lorentz Invariance with Gamma-Ray Burst Spectral-lag Measurements. Gamma-ray bursts (GRBs) are among the most potent probes of Lorentz invariance violation (LIV), offering direct constraints on the quantum gravity energy scale (EQG) based on observations of energy-dependent time lags. Individual GR... | [
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Plasma Characteristics of Active Region Footpoints before Eruptive and Confined Flares. Solar flares are powerful, explosive events that occur in solar active regions (ARs). They are typically classified as either eruptive or confined, depending on whether they are associated with coronal mass ejections. While many stu... | [
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Forging Neon-distilling White Dwarfs in the Stellar Engulfments of Helium White Dwarfs. Once carbon─oxygen white dwarfs cool sufficiently, they crystallize from the inside out. If the white dwarf is rich enough in 22Ne, these crystallized solids are buoyant and rapidly rise, efficiently liberating potential energy, whi... | [
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The Growth of the Central Black Holes in Quasi-stars. Observations by JWST have confirmed the presence of supermassive black holes (BHs) at redshifts z ≳ 10, lending support to scenarios in which BHs experience rapid growth through intense gas accretion. Here we investigate the growth of a BH embedded at the center of ... | [
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The Most Probable Behavior of the Dark Energy Equation of State Indicates a Thawing Quintessence Field: Tomographic Alcock─Paczyński Test with Redshift-space Correlation Function II. We apply an extended Alcock─Paczyński (AP) test to the Sloan Digital Sky Survey data to constrain the dark energy models with the Chevall... | [
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Probabilistic Interpolation of Sagittarius A*'s Multiwavelength Light Curves Using Diffusion Models. Understanding the variability of Sagittarius A* (Sgr A*) requires coordinated, multiwavelength observations that span the electromagnetic spectrum. In this work, we focus on data from four key observatories: Chandra in ... | [
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CORINOS. IV. Quantifying Baseline-fitting Uncertainties in SO<SUB>2</SUB> Ice Measurements with JWST/MIRI. Sulfur dioxide (SO2) ice has been tentatively detected in protostellar envelopes, but its reliability as a solid-state sulfur reservoir remains unclear. We present new measurements of SO2 ice from 6.8─8.5 μm towar... | [
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DESI Strong Lens Foundry. I. HST Observations and Modeling with GIGA-Lens. We present the Dark Energy Spectroscopic Instrument (DESI) Strong Lens Foundry. We discovered ∼3500 new strong gravitational lens candidates in the DESI Legacy Imaging Surveys using residual neural networks (ResNet). We observed a subset (51) of... | [
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Mass─Radius Constraints for 2S 0918─549 from an RXTE Superexpansion Burst: A Direct Cooling-tail Analysis. Thermonuclear (Type I) X-ray bursts from accreting neutron stars (NSs) offer a means to determine NS mass (M) and radius (R) and thereby probe the properties of matter at supranuclear density. A subset of these ev... | [
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JWST Observations of Cosmic-Ray-excited H<SUB>2</SUB> in Barnard 68: Spatial Variations and Constraints on Cosmic-Ray Attenuation. We present James Webb Space Telescope (JWST) NIRSpec observations of the starless dark cloud Barnard 68 (B68) that reveal the spatially resolved signature of cosmic-ray-excited molecular hy... | [
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Investigating Enols Chemistry in the Interstellar Medium: Rotational Spectroscopy and Interstellar Search of (E)-1-Propenol. Enols represent highly reactive intermediates toward the synthesis of complex organic molecules in the interstellar medium (ISM) and serve as key tracers of nonequilibrium chemistry driven by Gal... | [
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Fragmenting Filaments and Evolving Cores—Insights from Dust Polarization Study of a Filament in Northern Orion B. We present an analysis of polarized dust emission at 850 μm for a parsec-long filament in the northern part of the Orion B molecular cloud. The region was observed by the James Clerk Maxwell Telescope SCUBA... | [
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Laboratory Modeling of Supernova Remnants Collisions: Implications for Triggered Star Formation. Theoretical models of star formation consistently underestimate the rates observed in astronomical surveys. Stars form within giant molecular clouds, which fragment into dense clumps under the combined influences of turbule... | [
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3D MHD Simulations of Coronal Loops Heated via Magnetic Braiding. I. Continuous Driving. The nature and detailed properties of the heating of the million-degree solar corona are important issues that are still largely unresolved. Nanoflare heating might be dominant in active regions and quiet Sun, although direct signa... | [
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"http://astrothesaurus.org/uat/1483",
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3D MHD Simulations of Coronal Loops Heated via Magnetic Braiding. II. Automatic Detection of Reconnection Outflows and Statistical Analysis of Their Properties. Recent observations of fast and bursty "nanojets" suggest novel diagnostics of nanoflare heating in the solar corona. The aim of this work is to investigate th... | [
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Noisy Timing Behavior is a Feature of Central Compact Object Pulsars. We present a timing study of the three known central compact object (CCO) pulsars, isolated cooling neutron stars in supernova remnants, using observations from Chandra, XMM-Newton, and NICER spanning two decades. Relative to canonical young pulsars,... | [
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Testing the Shock-cooling Emission Model from Star─Disk Collisions for Quasiperiodic Eruptions. Quasiperiodic eruptions (QPEs), the repeated outbursts observed in soft X-ray bands, have attracted broad interest, but their physical origin is under debate. One of the popular models, the star─disk collision model, suggest... | [
"http://astrothesaurus.org/uat/1852",
"http://astrothesaurus.org/uat/1663",
"http://astrothesaurus.org/uat/1696"
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"http://astrothesaurus.org/uat/2086",
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Circumbinary Disks in Post Common Envelope Binary Systems with Compact Objects. We conduct a population synthesis study using the binary population synthesis code COMPAS to explore the formation of circumbinary disks (CBDs) following the common envelope evolution (CEE) phase of a giant star and a neutron star (NS) or b... | [
"http://astrothesaurus.org/uat/1108",
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Galactic-scale Quasar Pairs from the Sloan Digital Sky Survey and Gaia DR3. We perform a systematic search for galactic-scale quasar pairs and small-scale (<3″) lenses using the Sloan Digital Sky Survey (SDSS) DR16 quasar catalog and Gaia DR3, and identify 136 double quasar candidates from 1120 Gaia-resolved pairs a... | [
"http://astrothesaurus.org/uat/406",
"http://astrothesaurus.org/uat/159",
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The Maximum Gravity Model for Partial Tidal Disruption Events: Mass Loss, Peak Fallback Rate, and Dependence on Stellar Properties. A star entering the tidal sphere of a supermassive black hole (SMBH) can be partially stripped of mass, resulting in a partial tidal disruption event (TDE). Here, we develop an analytical ... | [
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COBIPLANE: A Systematic Search for Compact Binary Millisecond Pulsars at Low Galactic Latitudes. We present the main results obtained from the Compact Binary Pulsar Search in the Low-Latitude Neighborhood, an optical photometric survey designed to find new "spider" binary millisecond pulsars. We conducted observations ... | [
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Hint of Dark Matter─Dark Energy Interaction in DESI DR2 and Current Cosmological Dataset?. We present new constraints on an interacting dark matter─dark energy scenario motivated by string compactification, where a scalar field adiabatically tracks the minimum of an effective potential sourced by dark matter density. I... | [
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