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Millimeter Continuum Measurements of Circumstellar Dust Around Very Young Low Mass StarsWe investigate the question of disk formation during the protostar phase. We build on the results of Keene and Masson (1990) who analysis of L1551 showed themillimeter continuum emission comes from both an unresolved circumstellar conponent i.e. disk and an extended cloud core.
Document ID
20060038726
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/34977
Authors
Terebey, S.
Chandler, C. J.
Andre, P.
Date Acquired
August 23, 2013
Publication Date
December 1, 1992
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other
Keywords
dust continuum emission cloud core Owens Valley Interferometer data T Tauri phas

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