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The dust debris around HR 4796The IRAS data strongly suggest that there is dust debris around the main-sequence A star HR 4796. The optical depth of the dust cloud around HR 4796 is probably twice that around Beta Pic, the main-sequence star in the Bright Star Catalog which was previously thought to have the most opaque dust debris cloud.
Document ID
19920035453
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/186246
Authors
Jura, M. (California, University Los Angeles, United States)
Date Acquired
August 15, 2013
Publication Date
December 20, 1991
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 383
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
92A18077
Distribution Limits
Public
Copyright
Other

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