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- Effects of Resolution and Local Stability on Galactic Disks: I. Multiple Spiral Mode Formation via Swing Amplification
- How dust particles orbiting white dwarfs can reveal undetected co-orbiting exoplanets
- Magnetic field morphology and strength in the high-mass star-forming clump G31.41+0.31
- Persistent Sub-MeV Ion Enhancement Downstream of an Interplanetary Shock: Multispacecraft Observations near L1
- Optical Constants of Photochemical Haze Analogs in N ₂ –CH ₄ –CO Atmospheres from 0.4 to 28.6 μ m
- NuGNN: A Graph Neural Network for Nuclear Reaction Network Equations
- The JWST Weather Report from the Nearest Brown Dwarfs. III. Heterogeneous Clouds and Thermochemical Instabilities as Possible Drivers of WISE 1049AB's Spectroscopic Variability
- The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b
- A Cassini/CAPS Survey of Ionospheric Outflow at Saturn and Its Internal and External Drivers
- Insights into the Micromechanical Properties of Different Planetary Bodies: Nanoindentation Studies of Martian Olivines and Pyroxenes
- A Global Magnetohydrodynamic Simulation of the Birth and Cannibalism of Homologous Coronal Mass Ejections
- Filament-Arm Node Systems (FANS): A New Probe of the Winding and Chirality of the Cosmic Web
- A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b’s Panchromatic Spectrum
- No Strong Evidence for Plasma Lensing in FRB 20240114A
- A Collapsar-disk Origin for GW190814
- JWST Reveals a Highly Ionized Nebula Powered by an Ultraluminous X-Ray Source with a Massive Black Hole in the Metal-poor Galaxy Holmberg II
- Black Hole Binary Mergers in Galactic Nuclei: Combined Effects of Secular Dynamics and Stellar Flybys
- Moment-based Formulae for the Transport Coefficients
- The Effect of Adiabatic Index on Radius Evolution and the Mass Loss
- Turbulent Viscosity in Line-driven Stellar Winds
- Capturing Statistical Isotropy Violation with Rotational Averages
- Pressure–Strain Channels in Interchange Reconnection Simulation and Comparisons with MMS Observations
- X-reconstruction: 3D Tomographic Reconstruction in Astrophysics. I. Mathematical Formulation for Systems in the Optically Thin Regime
- How Eccentric is the Debris Disk of ϵ Eridani? ALMA Reveals a Near-circular Belt
- Mitigating the Timing Impact of Anomalous Pulse Profile Shape Variability in PSR J1713+0747 with Gaussian Component Modeling