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Analytic pulsar modelsAn analytical procedure is given for solving the Einstein equations of a rotating fluid body. It is demonstrated that an analytic model of uniform denisty, representing a slowly rotating neutron star, can describe both differentially and uniformly rotating stars.
Document ID
19740061137
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/153085
Authors
Adams, R. C.
Cohen, J. M. (Pennsylvania, University Philadelphia, Pa., United States)
Adler, R. J. (Institute for Advanced Study, Princeton, N.J.; NASA, Ames Research Center Moffett Field, Calif., United States)
Sheffield, C. (Earthsat Corp. Washington, D.C., United States)
Date Acquired
August 7, 2013
Publication Date
September 1, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 192
Subject Category
Space Sciences
Accession Number
74A43887
Distribution Limits
Public
Copyright
Other

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