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The jet model of chondrule formationWe estimate the size range of particles that are ejected from a protostellar accretion disk by a protostellar jet. An n-body code is used to determine the subsequent motion of the ejected particles, where the particles are subject to two forces: the gravitational attraction from the protostar; and the gas drag from the halo gas of the accretion disk.
Document ID
19950012895
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Liffman, K. (Commonwealth Scientific and Industrial Research Organization Highett, Victoria, Australia)
Date Acquired
September 6, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Lunar and Planetary Inst., Papers Presented to the Conference on Chondrules and the Protoplanetary Disk
Subject Category
Astrophysics
Accession Number
95N19310
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19950012874Collected WorksPapers presented to the Conference on Chondrules and the Protoplanetary Disk
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