Accretion and jet simulations in YSOs

• Type: Article in International Conference Proceedings Book
• Date: 2017

Authors

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

Conference proceedings International

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

Pages: 816-817

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

5 June 2017 through 9 June 2017

Indexing

Scopus - 1 Citation

Other information

Authenticus ID: 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.

Language: English

Type (Professor's evaluation): Scientific