Solar & stellar physics
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- Thermal Stability of Radiation-pressure-dominated Accretion Disks Threaded by Net Vertical Magnetic Flux
- Short-term solar flare forecasting with a hybrid ConvNeXtV2 and transformer–temporal convolutional network
- Thermodynamic and structural properties of the thin atmosphere of a white dwarf
- The formation of silicon-carbon chain molecules in IRC+10216
- Heating of Solar Coronal Loops by Converging Unipolar Magnetic Flux: Evidence from SDO Observations and a Radiative MHD Simulation
- Periodic radio emission from a rapidly rotating T8 ultracool dwarf
- Calculation of distant retrograde orbits and their use in space weather forecasting
- Dynamical plausibility of triple-assisted interaction in Be-star multiple systems
- Reduced magnetohydrodynamics with electron inertia in pseudodipole coordinates
- Testing Pre-main-sequence Evolutionary Models with Gaia and SPHEREx Observations of Canis Major North
- DUETS II - Red giant asteroseismic binaries. Binary confirmation and prospects for double-seismic model inference
- A Model to Map Brown Dwarf Companions to White Dwarfs in Partial Secondary Eclipse
- The evolutionary history of ultra-compact accreting binaries. II. HST spectroscopy of two eclipsing AM CVn stars
- An intermediate-mass stripped star with a dark companion in the Small Magellanic Cloud
- The Stellar Populations of Resolved Galaxies
- How Common Are Common Envelopes? Quantifying Their Role in Forming Gravitational-Wave Sources
- Direct measurement of the 23Mg(p, γ)24Al reaction using the DRAGON recoil separator and a hybrid array of γ-ray detectors
- The Impact of Flyby Interactions on the Rotation of Open Clusters
- Connectivity rewiring and filament formation by active region emergence observed with Solar Orbiter
- Scale-Dependent Statistics of Coherent Magnetic Structures in Early IMAP Observations
- The mass discrepancy problem in massive stars: an inferential perspective
- Explainable Prediction of High-Speed Solar Wind Streams driven by Coronal Holes via Topological Data Analysis
- An Intermediate Mass Stripped Star in a 4.2-hour Orbit around a Compact Object
- Physical assumptions versus nature: the shape of the heliosphere
- Delayed maximum energy solar energetic particle events: Statistical analysis from Solar Orbiter