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A radiation-driven disc wind model for massive young stellar objects
Home
Publications
A radiation-driven disc wind model for massive young stellar objects
A radiation-driven disc wind model for massive young stellar objects
Authors:
Janet E. Drew
Janet E. Drew
Daniel Proga
Daniel Proga
JS
James M. Stone
James M. Stone
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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
DOI:
10.1046/j.1365-8711.1998.01438.x
Abstract
No abstract available
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)
Cited
Cited by 44 articles
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