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Binary and Millisecond Pulsars

Phinney, E. S. and Kulkarni, S. R. (1994) Binary and Millisecond Pulsars. Annual Review of Astronomy and Astrophysics, 32 . pp. 591-639. ISSN 0066-4146. http://resolver.caltech.edu/CaltechAUTHORS:20120223-080709481

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Abstract

Most of the ~600 known pulsars are single and located in the disk of our Galaxy. There is circumstantial evidence that the pulsars in this majority are created in supernova (SN) explosions, by the collapse of the cores of massive stars (initial mass M_i ≳ M_(cr) ≃ 8 M_⊙). One is created roughly every 100 y in the Galaxy.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1146/annurev.aa.32.090194.003111DOIArticle
http://www.annualreviews.org/doi/abs/10.1146/annurev.aa.32.090194.003111PublisherArticle
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Additional Information:© 1994 by Annual Reviews Inc. ESP was partly supported by NASA Astrophysics Theory grant NAGW-2394 and the Alfred P. Sloan Foundation. SRK’s work was supported by NASA, NSF, and the Packard Foundation.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NASANAGW-2394
Alfred P. Sloan FoundationUNSPECIFIED
NSFUNSPECIFIED
David and Lucile Packard FoundationUNSPECIFIED
Record Number:CaltechAUTHORS:20120223-080709481
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120223-080709481
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:29424
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Feb 2012 19:54
Last Modified:30 Oct 2017 23:08

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