Solar & stellar physics
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- The origin of UV emission in extremely low-mass satellite galaxies: Insights from Leo T
- Periodic activity on the (sub)millimetre surface of the asymptotic giant branch star Mira A
- Diversity of planetary origins and compositions traced by stellar abundance differences among co-natal star systems
- Size, atmospheric, and ring constraints on the large Kuiper belt object (55565) Aya from a stellar occultation
- UOCS. XVI. Census of post mass-transfer binaries across various evolutionary phases in M67
- Evolution and Geometry of the Heliotail across 14 yr of IBEX-Hi Observations (2009–2022): A Baseline for IMAP-era Heliotail Studies
- A Search for Dust in the Outflow of the HH 212 Class 0 Protostellar System
- Improved Astrometry in a Sparse Star Field and New Positions of Triton and Nereid (2018–2020)
- An Updated Model for ϵ Eridani b and Prospects for Imaging with the Roman Coronagraph
- POSEIDON. III. The Aligned Orbit of the Hot Neptune around the Hot Star WASP-195
- Radiation Magnetohydrodynamic Simulation of Sub-Eddington Circumbinary Disk in a 10:1 Massive Black Hole Binary
- Perpendicular Heating of Solar Wind Protons Driven by Proton Cyclotron Waves Upstream of Mars
- A New Framework for Modeling Solar Flares from Magnetohydrodynamic to Kinetic Processes
- Eight Gamma-Ray Bursts Observed with the Fermi Gamma-Ray Burst Monitor: Significant Quasi-thermal Components and Conditional Jet Constraints
- Impact of Upstream Clumpiness on Supernova Remnant Forward Shock Evolution in Molecular Cloud Environments
- Joint Multiband Photometry with crowdsource
- An Exploration of In-band Spectral Index Techniques for Extended Radio Sources with EMU
- Coevolution of Dust Growth and Gravitational Instability in Massive Protostellar Disks
- Stellar Collisions from Self-consistent Stellar Dynamics around Growing Supermassive Black Holes
- Planetary Accretion Is Less Frequent in Wide Binaries: Evidence from Metal-enriched White Dwarfs in DESI DR1
- Damping and Dispersion of Acoustic Waves in the Solar Corona
- Two-Fluid Radial Stability of Dark-Matter-Admixed Compact Objects: Dark Compact Planets, Dark White Dwarfs, Dark Neutron Stars, and Dark Oysters
- Equipartition between Alfvénic turbulence and energetic ions as the origin of the -5 common spectrum in the heliosphere
- The Importance of Curium-250 to the γ-Ray Signature of r-Process Remnants
- Likely Metal Scarring in the Magnetic White Dwarf LHS 2534