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 News from astronomynow.com

› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
› Dark matter may come in multiple forms, new model suggests
› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
› XRISM solves gamma-Cas’s 50-year X-ray mystery
RSS  Latest preprints on astro-ph:

› Effects of Pebble Accretion Isolation Mass on Observable Exoplanet Properties
› Laser Metrology for Precision Alignment of Transmission Gratings in the REDSoX Soft X-ray Polarimeter
› Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. III. Mass Distribution of Hierarchical Mergers
› Explosions from Rotating Very Massive Star Collapses to Black Holes: Effects of Nuclear Burning
› Observational Constraints on Horizonless Compact Objects from Thermal Emission in AGNs
› A binary black hole merger rate comparison within the same metallicity - star formation rate framework
› Radio Properties of RS Canum Venaticorum Variables in VLASS and RACS
› No Evidence for Nearby Circumstellar Material in the Type Ia Supernova 2025rbs
› Abundant Heavy Black Hole Seeds from Moderate Lyman-Werner Radiation
› High-Energy Neutrinos from Supernova Shock Breakouts in Circumstellar Media: Light Curves, Spectra, and Contribution to the Extragalactic Neutrino Background
› The second Arcminute Microkelvin Imager -- Large Array Gamma-ray burst radio afterglow catalog
› Old Disks Die Hard: How Does AGN Feedback Suppress Disk Formation in Milky Way Mass Galaxies?
› MORFEO control strategy
› The CMZ Asymmetries: Feeding or Feedback?
› Performance Analysis of the Asgard/NOTT Nulling Interferometer: Optimizing Observing Modes for High-contrast Detection
› H-$\alpha$ Integral Carrington Synoptic Maps Produced by NSO/NISP
› Time-dependent multi-energy neutrino emission from symbiotic recurrent novae: the role of accretion disks
› Energy Partitioning in Dust-catalyzed $\mathrm{H_2}$ and HD Formation Revealed by Molecular Simulations Considering Nuclear Quantum Effects
› CCAT: a two-octave 1.024 GHz KID readout featuring an overlap-channel polyphase synthesis filter bank on RFSoC
› Enhancing the performance and capabilities of the MIRI instrument on JWST
› A chemo-dynamical search for planet-candidate hosts of possible extragalactic origin
› Evidence for Dynamical Filtering: High Binary Fraction, Hard-binary Excess, and Unresolved Triples in the Surviving Core of NGC 6791
› On the Acceleration of Pulsar Timing computations using Normalising Flows and Parallelisation
› How mergers shape galaxy morphology in the IllustrisTNG simulation
› X-ray Activity of the RS CVn-type Star {\sigma} Gem with the First-Year Observations of Einstein Probe
› Detection of possible burst oscillation in the neutron star low-mass X-ray binary 4U 1323-62
› The SAMI Galaxy Survey: Linking Tidal Features and Orbit Populations Using Schwarzschild Modelling
› The galaxies' energy balance problem solved
› High-order Paschen emission from the quiet-Sun off-limb chromosphere
› Aether.jl : A High-Performance 3D MHD and Multifluid Dust Code Written in a Dynamic Language with an Interactive Human-AI Development Framework
› The B-Index as a Diagnostic of Cool Stars: Assessing Metallicity Dependence of TiO Absorption in the Visible Spectrum
› A Reproducible Two-Boundary Kinematic Correction for Baryonic Rotation-Curve Reconstruction in an 84-Galaxy SPARC Benchmark
› Constraining Primordial Power Asymmetry from Galaxy Clustering and Peculiar Velocity Information
› Cosmographic Reconstruction of the Quintessence Potential in Scalar-Tensor Gravity
› Magnetoacoustic Portals in Quiet-Sun Fluxtubes Revealed by Chromospheric Spectropolarimetry with SUNRISE III/SCIP
› Launching Jets in Tidal Disruption Events: Magnetic Flux Advection and Plasma Loading
› Cosmicflows-4 and the Cosmological Consistency of Large-Scale Motions
› The Evolution of the ACIS Contamination Layer on the Chandra X-ray Observatory from 2010 to 2026
› The Galactic Centre G+0.633-0.0604 Molecular Cloud: A New Gold Mine for Astrochemistry
› Optical Spectroscopy of TeV-emitting BL Lac Candidates
› XRISM reveals sloshing-driven gas motions in the core of Abell 2029
› How X-rays heat the IGM in different 21-cm simulation codes: a comparison between Licorice and Beorn
› OH Line Detections in Southern Galaxies of the IRAS Revised Bright Galaxy Sample
› The deepest color-magnitude diagrams for the benchmark open cluster NGC 2437 from Gaia and VVVX
› Hydrogen Engulfment into Sub-Neptune Cores through Magma Ocean Convective Surface Renewal
› ATLAS. IV. A JWST+MUSE Demographic Study of Ly$\alpha$ Profiles in Little Red Dots
› Cosmic Ray Diffusion and the Origin of Very High Energy Gamma-Ray Emission in Young Massive Stellar Clusters
› High-Frequency Thermal Noise in Michelson Interferometers
› Unknown Unknowns: Model Misspecification in Machine Learning for Physics
› From the Earth to the Sun
› Quasinormal modes as exterior probes of black hole interiors in our Universe
› Axion Isocurvature Perturbations Survive the Scaling Evolution of Axion Domain Walls
› Gravitational Waves from Dimension-6 Assisted Peccei - Quinn Phase Transitions
› Altitude-Dependent Near-Source Spectral Filtering of Meteor Infrasound Above 80 km and Consequences for Period-Based Energy Estimates
› Physics of Circular Polarized Ion-Scale Waves in Hybrid Simulations of Alfv\'enic Fluctuations
› Blazar Boosted Dark Matter in IceCube
› Multivariate time series transformer embeddings for light curves of periodic variable stars
› Identifying galactic binary systems of neutron stars and black holes with LISA
› Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data
› Stability Boundary of Neutron-Dark Matter Mixed Stars
› Beyond Sgr A* and M87*: Sub-Microarcsecond Black Hole Shadow Detection via Lunar-based Extremely Long Baseline Interferometry
› Distinguishing the nature of dark matter by mapping cosmic filaments from Lyman-alpha emission
› Inferring population III star properties from the 21-cm global signal
› Analysis of the Space Velocities of Several Samples of Open Star Clusters
› Pulsar scintillation arcs formed from correlated volume scattering
› Short-Range Forces Can Catalyze Extreme Orbital Evolution in Hierarchical Triples
› 3D Kinematic Reconstruction of the Crab Nebula That Includes the Northern Ejecta `Jet'
› Prediction for IMAP: Revealing the Role of the Solar Magnetic Field in the Heliotail
› The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654
› The incidence of eROSITA X-ray AGN in the local Universe: from dwarf to massive galaxies
› Environmental dependence of Type Ia supernova standardization on the local luminosity-weighted age
› Three-Dimensional Dust Distribution in the Jovian System from Juno/Waves Observations: Insights into the Halo Ring and Magnetospheric Dust
› Hubble tension: a short review of theoretical explanations
› eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge
› GLOW II: A Census of Oxygen in Low-Mass Galaxies
› A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution
› Synchrotron and Inverse-Compton Signatures of Black to White Hole Explosions: Weibel-Mediated External Shocks in the Interstellar Medium
› SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$
› Assessing Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, $\gamma$ Leo
› NuOscProbExact: a fast, general-purpose code to compute exact two-, three-, and four-flavor neutrino oscillation probabilities
› Achromatic, spin-odd Kerr EVPA as a null Frenet-Serret torsion integral on the photon ring
› Revisiting $^7$Be Weak and Radiative Transition Rates in Big Bang Nucleosynthesis: Implications for the Primordial Lithium Problem
› Phase Transitions and Gravitational Waves
› Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars
› Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions

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