Accretion and jet simulations in YSOs

• Tipo: Artigo em Livro de Atas de Conferência Internacional
• Data: 2017

Autores

Sauty, C (Autor) Outra; Cayatte, V (Autor) Outra; Tsinganos, K (Autor) Outra; Lima, JJG (Autor) FCUP; De Albuquerque, RMG (Autor) Outra; Gameiro, JF (Autor) FCUP

Ata de Conferência Internacional

Título: Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society

Páginas: 816-817

2017 Conference Francesco's Legacy: Star Formation in Space and Time

5 June 2017 through 9 June 2017

Indexação

Scopus - 1 Citação

Outras Informações

ID Authenticus: P-00N-XNH

Abstract (EN): We have performed numerical simulations with the PLUTO numerical code starting from the analytical MHD model for RY Tau of Sauty et al.. We model the circumstellar corona with a stellar jet, surrounded by a magnetospheric accretion zone, an equatorial static dead zone and an external disk wind. The simulation attains a steady or quasi steady state in a few stellar rotations. Sporadic coronal mass ejections are present only if the mass accretion rate is much larger than the stellar mass loss rate. © SAIt 2017.

Idioma: Inglês

Tipo (Avaliação Docente): Científica