Effects on v sin i determinations of O stars from 3D model atmospheres with high turbulent velocities

Context. When studying massive stars and their life cycles, rotation plays a key role. Hence, understanding the rotation of these stars is crucial when determining their properties, or for constraining evolutionary models. Aims. We examined the reliability of the standard methods to derive projected...

Celý popis

Podrobná bibliografie

Hlavní autoři:	Delbroek L., Sundqvist J. O., Backs F., Ceulemans T., Debnath D., Schillemans P.
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2026-06-01
Edice:	Astronomy & Astrophysics
Témata:	hydrodynamics radiative transfer methods: numerical stars: atmospheres stars: massive stars: winds outflows
On-line přístup:	https://www.aanda.org/articles/aa/full_html/2026/06/aa60102-26/aa60102-26.html
Tagy:	Přidat tag Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!