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The rotation curve conspiracy and neutron star/asteroid models for Gamma Ray BurstsGamma Ray Bursts (GRB) were analyzed using new GRO/BATSE results in conjunction with older PVO and KONUS data. It is suggested that the distribution in space of the GRB sources must have an outer bounding surface which is approximately a sphere centered on the location. Neutron stars in some kind of extended halo around the Galaxy with the required mass of an infalling object of order about 10 exp 21 to 10 exp 23 gm are considered.
Document ID
19930052457
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Salpeter, Edwin E. (NASA Headquarters Washington, DC United States)
Wasserman, Ira (Cornell Univ. Ithaca, NY, 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
Astronomy
Accession Number
93A36454
Funding Number(s)
CONTRACT_GRANT: NAGW-666
CONTRACT_GRANT: NSF AST-89-13112
Distribution Limits
Public
Copyright
Other

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IDRelationTitle19930052429Collected WorksPlanets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992
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