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Mass loss rates from protostars and OI(63 micron) shock luminositiesThe high-velocity ejection of material from protostars results in a wind shock which may be observable in OI(63 micron) emission. It is shown that for a wide range of conditions, the OI(63 micron) luminosity is proportional to the mass loss rate from the protostar. Application is made to shock OI(63 micron) emission observed around IRc2 in the BN-KL region of Orion.
Document ID
19850042604
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hollenbach, D.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Icarus
Volume: 61
ISSN: 0019-1035
Subject Category
Astrophysics
Accession Number
85A24755
Funding Number(s)
CONTRACT_GRANT: NASA TASK 188-41-53-06
Distribution Limits
Public
Copyright
Other

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