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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1583

Title: The pulsar velocities and their binary origins (Invited review)
Authors: Radhakrishnan, V.
Shukre, C.S.
Keywords: BINARY STARS,
PULSARS,
STELLAR EVOLUTION,
STELLAR MOTIONS,
EXPLOSIONS,
NEUTRON STARS,
STELLAR ENVELOPES,
STELLAR MASS,
STELLAR ORBITS
Issue Date: Jan-1986
Publisher: D. Reidel Publishing Co.
Citation: Astrophysics and Space Science, 1986, Vol.118, p329-336
Abstract: The observed proper-motions are shown to indicate that most pulsars come from binary systems. Due to a remarkable relationship between the speed of a pulsar and that of its progenitor in orbit, it is concluded that these binaries went through a common-envelope phase. This provides independent support to similar conclusions drawn from stellar evolution consideration.
Description: Paper presented at the Third Asian-Pacific Regional Meeting held in Kyoto, Japan, Sept. 30-Oct. 6, 1984. Restricted Access. Open access version available at the alternative location.
URI: http://hdl.handle.net/2289/1583
ISSN: 0004-640X
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1986Ap&SS.118..329R
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986Ap%26SS.118..329R&link_type=ARTICLE&db_key=AST
Copyright: (1986) D.Reidel Publishing Co.
Appears in Collections:Research Papers (A&A)

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