A radiation-driven disc wind model for massive young stellar objects

• 1 May 1998
• journal article
• research article
• Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
• Vol. 296  (1) , L6-L10
• https://doi.org/10.1046/j.1365-8711.1998.01438.x

Abstract

Keywords

• HYDRODYNAMICS
• ACCRETION DISCS
• STARS:MASS-LOSS
• STARS: PRE-MAIN SEQUENCE
• YOUNG STELLAR OBJECT
• WIND SPEED
• ACCRETION

All Related Versions

• Version 1, 1998-01-06, ArXiv (Unconfirmed version)