Solar & stellar physics
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- The Role of Small-scale Environments in the Quenching of Massive Galaxies at 1 < z < 5
- Unified Scaling Relation for Coronal Temperature Anomaly and Solar Wind Acceleration
- The influence of dust composition on accretion outbursts
- A MUSE study of stellar and ionized-gas kinematics in central group galaxies
- The PLATO Input Catalog of targets (tPIC) for the first Long-duration Observation Phase field
- An extended red wing of the 5797 Å diffuse interstellar band in the Red Rectangle nebula
- The upper main sequence in h and ̧hi Persei
- Evidence for a nova super-remnant surrounding the recurrent nova V745 Scorpii using eROSITA
- VLT/X-Shooter spectroscopic characterisation of the Didymos system, target of the ESA Hera mission
- Nongravitational motion of 3I/ATLAS far from the Sun: robust detection, weak constraints on the activity law
- Stellar bars reshape the spatial distribution of UV-bright clumps in nearby galaxies
- Unsupervised selection and characterisation of little red dots in JWST surveys with manifold learning
- Tighter dark-matter constraints from the projected mass method: A neural-network-enhanced method for galaxy groups and clusters
- Characterising the O9–B1 spectral transition in the near-infrared
- Perpendicular transport in isotropic magnetic turbulence. The role of stochastic drifts
- The origin and distribution of diffuse HI in the close interacting MHONGOOSE galaxy systems
- Paschen jumps in little red dots: Evidence of nebular continua
- Hi intensity mapping with MeerKAT: A measurement of the 21-cm auto-spectrum on cosmological scales
- The ASPIICS solar coronagraph aboard the Proba-3 formation flying mission
- The imprint of individual neutron star spins on ejecta, r -process nucleosynthesis, and kilonovae in binary neutron star mergers
- Temperature-dependent differences between empirical lithium age estimators in benchmark open clusters
- How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations
- Structural composition and atmospheric analysis of two planetary systems : TOI-270 and TOI-776
- Trapped sausage modes in magnetic pores: existence criteria and viscous damping
- A VLT/CRIRES+ study of helium 1.083μm absorption features towards the inner Orion Nebula