Diagnosis of stellar winds and temperature structures in Be stars through the analysis of Mg II lines
Artículo
Acceso abierto
Artículo
SEDICI UNLP
We compute non-LTE Mg II line profiles for Be stars by considering 12 energy-level atoms and supposing that the circumstellar medium can be described by an expanding, spherically symmetric flow in which we assume the pre...
Idioma en
Acceso abiertoRuta libre sin proxy. Acceso recomendado cuando no hay suscripción activa.
Open Access