Solar & stellar physics
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- Supergranulation as a Tracer of Solar-Cycle Variability
- Stability of circumbinary planets: The role of binary properties and migration scenarios
- The δ Scuti instability strip and period-luminosity relation as seen by TESS and Gaia DR3
- On the Proper 3D Modeling of Orbits in Wide Binary Gravity Tests
- Extension and validation of the ZPEKTR code for determining the inclination angles of Be stars
- Six New Eclipsing AM CVn Binaries from the Zwicky Transient Facility
- Playing CHESS with stars II. Homogeneous analysis of high-resolution optical spectra for a sample of 135 giants in 14 bulge globular clusters
- Cascade models of anisotropic turbulence in magnetized plasma of solar wind
- Evolution of Binaries Under Stochastic Perturbations
- Nine new eclipsing accreting ultracompact white dwarf binaries from the Zwicky Transient Facility
- Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. IV. Heavy Element Enhanced Stars
- Analysis of Multi-Wavelength Data for 30 Galactic Emission-Line Stars with Dusty Envelopes
- Recent advances in numerical modeling of solar inertial modes
- Energy-Dependent Hard X-Ray QPP Modulation in M- and X-Class Solar Flares Observed by Aditya-L1/HEL1OS
- The first mass peak of merging black holes from core binding energies and jet-driven explosions
- Detection of HNCOH+ in the interstellar medium
- The Pointing Error Due To Laser Propagation in Space Plasma for TianQin Gravitational Wave Detection
- Insights into the Kinematic Evolution of Filament-Induced Jets: Coupling of Interchange and Flare Reconnection
- A Low-Dimensional Chemical Representation of High-Resolution Stellar Disk Spectra: Residual Abundance Signatures
- Operating the Fabry-Pérot systems of the European Solar Telescope in multi-aperture mode
- Two successive solar energetic electron events on 24 December 2022
- Rotation and outburst-like brightenings in ZZ Ceti stars observed by TESS
- Metal-poor molecular clouds in dwarf galaxies at parsec-scale resolution
- Mass-dependent multiplicity fraction in low-mass stars revealed by astrometry Gaia
- MAXI J1820+070: A rapidly rotating black hole with a mildly truncated disk and warm corona layers in the soft state