The pulsar velocities and their binary origins (Invited review)
| dc.contributor.author | Radhakrishnan, V | |
| dc.contributor.author | Shukre, C S | |
| dc.date.accessioned | 2006-12-14T07:51:47Z | |
| dc.date.available | 2006-12-14T07:51:47Z | |
| dc.date.issued | 1986-01 | |
| dc.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. | en |
| dc.description.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. | en |
| dc.format.extent | 752166 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Astrophysics and Space Science, 1986, Vol.118, p329-336 | en |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.uri | http://hdl.handle.net/2289/1583 | |
| dc.language.iso | en | en |
| dc.publisher | D. Reidel Publishing Co. | |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1986Ap&SS.118..329R | en |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986Ap%26SS.118..329R&link_type=ARTICLE&db_key=AST | en |
| dc.rights | (1986) D.Reidel Publishing Co. | en |
| dc.subject | BINARY STARS, | en |
| dc.subject | PULSARS, | en |
| dc.subject | STELLAR EVOLUTION, | en |
| dc.subject | STELLAR MOTIONS, | en |
| dc.subject | EXPLOSIONS, | en |
| dc.subject | NEUTRON STARS, | en |
| dc.subject | STELLAR ENVELOPES, | en |
| dc.subject | STELLAR MASS, | en |
| dc.subject | STELLAR ORBITS | en |
| dc.title | The pulsar velocities and their binary origins (Invited review) | en |
| dc.type | Article | en |