Dusty debris clouds around main sequence and post-main sequence starsDuring the past decade, infrared observations by IRAS and from the ground have revealed that many stars are orbited by dusty debris disks. Somewhat more indirect arguments indicate that many of these systems also contain asteroids, comets, and/or planets, thereby suggesting that planetary systems may be quite common in the Milky Way. Dust clouds at the main sequence K5 star HD 98800 and the white dwarf Giclas 29-38 are particularly noteworthy and mysterious.
Document ID
19930052452
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Zuckerman, B. (California Univ. Los Angeles, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36426 14-90)
Publisher: Astronomical Society of the Pacific
Subject Category
Astrophysics
Accession Number
93A36449
Distribution Limits
Public
Copyright
Other
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Related Records
IDRelationTitle19930052429Collected WorksPlanets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992