10.9k citations
- Centre National de la Recherche ScientifiqueFR5k papers
- Sorbonne UniversitéFR2.7k papers
- Délégation Paris 7FR2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2k papers
- CEA Paris-SaclayFR1.7k papers
- Astrophysique, Instrumentation et ModélisationFR1.2k papers
- Sorbonne Paris CitéFR1.1k papers
- Université Paris-SaclayFR1k papers
- Université Paris Sciences et LettresFR1k papers
- Observatoire de ParisFR994 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR986 papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR955 papers
584 papers · 1 filter
Chemical tracers of a highly eccentric AGB-main sequence star binary
T. Danilovich, J. Malfait, M. Van de Sande +32
Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB) stars and planetary nebul…
Imprint of the magnetic activity cycle on solar asteroseismic characterisation based on 26 years of GOLF and BiSON data
Jérôme Bétrisey, Martin Farnir, Sylvain N. Breton +4
Building on the success of previous missions, asteroseismic modelling will play a key role in future space-based missions, such as PLATO, CubeSpec, and Roman. Despite remarkable ac…
Magnetism in LAMOST CP stars observed by TESS
Keegan Thomson-Paressant, Coralie Neiner, Jonathan Labadie-Bartz
Context. A thousand new magnetic candidate CP stars have been identified with LAMOST, among which about 700 prime targets have rotational modulation determined from TESS. Aims. We…
Dust evolution during the protostellar collapse: influence on the coupling between the neutral gas and the magnetic field
Valentin Vallucci-Goy, Ugo Lebreuilly, Patrick Hennebelle
The coupling between the magnetic field and the gas during the collapsing phase of star-forming cores is strongly affected by the dust size distribution, which is expected to evolv…
Effect of Rotation on Wave Mixing in Intermediate Mass Stars
A. Varghese, R. P. Ratnasingam, R. Vanon +3
Internal gravity waves (IGWs) are likely to cause mixing in stellar interiors. Studies show that the mixing by these waves changes drastically across age and mass (Varghese et al.…
Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
A. R. G. Santos, D. Godoy-Rivera, A. J. Finley +4
While the mission's primary goal was focused on exoplanet detection and characterization, Kepler made and continues to make extraordinary advances in stellar physics. Stellar rotat…