The pulsar velocities and their binary origins (Invited review)

Details The pulsar velocities and their binary origins (Invited review) The pulsar velocities and their binary origins (Invited review)

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..329r&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Pulsars, Stellar Evolution, Stellar Motions, Explosions, Neutron Stars, Stellar Envelopes, Stellar Mass, Stellar Orbits

Scientific paper

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 considerations.

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