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Hydrogen flash in stars.The initial adiabat of the gas in a flat rotating disk is estimated in several ways. A star which can be represented by a polytrope of index 1.5 is considered. The central conditions are determined through specification of the total mass and the adiabatic constant. The values for the temperature and the density of the center are much higher than now exist at the center of the sun. It is possible that the ignition of hydrogen-burning reactions at the center of the disk can be accompanied by a thermal runaway.
Document ID
19730042773
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Perri, F.
Cameron, A. G. W.
(Yeshiva University; NASA, Goddard Institute for Space Studies, New York, N.Y., United States)
Date Acquired
August 7, 2013
Publication Date
April 6, 1973
Publication Information
Publication: Nature
Volume: 242
Subject Category
Space Sciences
Accession Number
73A27575
Distribution Limits
Public
Copyright
Other

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