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Planet formation around millisecond pulsarsWe present a model for the formation of planets in circular orbits around millisecond pulsars. We propose that the planets originate from a circumbinary excretion disk around a binary millisecond pulsar and show how physical conditions in such a disk lead to the eventual formation of planets.
Document ID
19930052442
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Banit, Menashe
(NASA Headquarters Washington, DC United States)
Ruderman, Malvin
(NASA Headquarters Washington, DC United States)
Shaham, Jacob
(Columbia Univ. New York, 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
93A36439
Funding Number(s)
CONTRACT_GRANT: NCC5-37
CONTRACT_GRANT: NAGW-1618
CONTRACT_GRANT: NSF AST-89-01681
Distribution Limits
Public
Copyright
Other

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