Solar & stellar physics
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- A Large-Sample Study of Interstellar Reddening in Galactic Star Clusters
- The Pristine survey XXXI. A stream offset from the Stream: very metal-poor stellar debris trailing 100∘ from the LMC-SMC system
- First Results from JACKS: A VLA Ammonia View of Gas Heating and Star-forming Cores in the Central Molecular Zone
- Systematic Search for Cataclysmic Variables in Radio Surveys: First Radio Detection of IX Velorum
- MP-DualNet: A Dual-Branch Deep Learning Approach for Magnetopause Boundary Detection Using Simulated SXI Images
- No Significant Rotation of the Spiral Structure in the IM Lup Protoplanetary Disk
- Double Neutron Star Mergers and Fast Blue Optical Transients: A Circumbinary Disk Connection
- FastChem 4: New chemical elements and improved convergence behaviour
- GWTC-4.0: Searches for Gravitational-wave Lensing Signatures
- Detection of Fine-structured Radio Bursts during a Superflare on EQ Peg
- Discovery of the redback pulsar PSR J2053+6905 and multi-epoch optical observations of the system
- Missing Outer Rings in the exoALMA Sample: Physical Mechanisms Suppressing Dust Ring Formation Despite Strong Pressure Bumps
- SDSS-V LVM: Revealing the Physical and Chemical Structure of the Helix Nebula
- The slower rotation of planet-hosting stars revisited
- Accretion-powered flares from black hole–disc collisions in galactic nuclei
- Forward-modelling the Tolman and distance-duality tests with IllustrisTNG
- EMU/GAMA: Understanding the link between dust geometry and star formation rate in galaxies
- Solar Wind Turbulence Spectra and Correlation Scale from 4 to 50 r ⊙: STEREO and PUNCH Observations
- Three-dimensional wave optics for weak-field lensing of gravitational waves
- Exploring Cosmological Tensions with Hubble Parameter Tomography
- Stellar bar occurrence in TNG50 and TNG100: disentangling environmental effects and assembly history at z = 0.
- Dispersion Measure Variability in Fast Radio Bursts from Photoionization
- Stationary Resistive MHD Solutions near an Isolated Three-dimensional Magnetic Null
- Multispacecraft Constrained Modeling of Solar Energetic Particle Transport across Different Heliocentric Radii and Heliolongitudes
- Estimates of Magnetic Field Strength in the Solar Corona Using Observations of Thermal Radio Emission at Low Frequencies