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Journal Articles Memorie della Societa astronomica italiana Year : 1970

Accretion and jet simulations in YSOs .

K. Tsinganos
  • Function : Author
J. J. G. Lima
  • Function : Author
J. F. Gameiro
  • Function : Author


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.
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obspm-04058769 , version 1 (05-04-2023)



C. Sauty, V. Cayatte, K. Tsinganos, J. J. G. Lima, R. M. G. de Albuquerque, et al.. Accretion and jet simulations in YSOs .. Memorie della Societa astronomica italiana, 1970, 88, pp.816. ⟨obspm-04058769⟩
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