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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1583
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dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorShukre, C.S.-
dc.date.accessioned2006-12-14T07:51:47Z-
dc.date.available2006-12-14T07:51:47Z-
dc.date.issued1986-01-
dc.identifier.citationAstrophysics and Space Science, 1986, Vol.118, p329-336en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2289/1583-
dc.descriptionPaper 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.en
dc.description.abstractThe 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.en
dc.format.extent752166 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.-
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1986Ap&SS.118..329Ren
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986Ap%26SS.118..329R&link_type=ARTICLE&db_key=ASTen
dc.rights(1986) D.Reidel Publishing Co.en
dc.subjectBINARY STARS,en
dc.subjectPULSARS,en
dc.subjectSTELLAR EVOLUTION,en
dc.subjectSTELLAR MOTIONS,en
dc.subjectEXPLOSIONS,en
dc.subjectNEUTRON STARS,en
dc.subjectSTELLAR ENVELOPES,en
dc.subjectSTELLAR MASS,en
dc.subjectSTELLAR ORBITSen
dc.titleThe pulsar velocities and their binary origins (Invited review)en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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