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Nonstandard thermal evolution of neutron starsA neutron star may cool much faster than through the 'standard' scenario. Here we calculate thermal evolution of neutron stars through various 'nonstandard' fast cooling scenarios, and the results are compared with the currently up-dated observational data. We discuss the possibility of distinguishing between the standard and various, different nonstandard scenarios, through the current and future X-ray satellite observations.
Document ID
19950038084
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/174641
Authors
Umeda, Hideyuki (Montana State Univ. Bozeman, MT, United States)
Tsuruta, Sachiko (Montana State Univ. Bozeman, MT, United States)
Nomoto, Ken'ichi (Univ. of Tokyo Tokyo, Japan)
Date Acquired
August 16, 2013
Publication Date
September 20, 1994
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 433
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
95A69683
Funding Number(s)
CONTRACT_GRANT: NAGW-2208
CONTRACT_GRANT: NSF AST-90-13290
Distribution Limits
Public
Copyright
Other

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