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On the orientation of the pulsar space velocity vector relative to the spin axis

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dc.contributor.author Kochhar, R. K
dc.date.accessioned 2009-02-03T13:55:27Z
dc.date.available 2009-02-03T13:55:27Z
dc.date.issued 1977-05
dc.identifier.citation Nature, Vol. 267, pp. 231 en
dc.identifier.issn 0028-0836
dc.identifier.uri http://hdl.handle.net/2248/4317
dc.description Restricted Access
dc.description.abstract It is noted that the angle between the space velocity vector and the spin axis projected on the plane of the sky has a value close to zero deg for three pulsars, close to 90 deg for six others, and between zero and 90 deg for two more. A hypothesis that could explain how these different orientations arose is presented which involves three modes of pulsar formation. It is suggested that pulsars formed in supernova explosions of single stars should have angles of approximately zero deg, that pulsars with angles close to 90 deg were liberated from binary orbits disrupted by supernova explosions of their companions, and that pulsars with angles between zero and 90 deg were produced by supernovae of their own progenitors in (subsequently disrupted) binary systems. en
dc.language.iso en en
dc.publisher Nature Publishing Group en
dc.relation.uri http://adsabs.harvard.edu/abs/1977Natur.267..231K en
dc.relation.uri http://dx.doi.org/10.1038/267231a0 en
dc.subject Axes of Rotation en
dc.subject Pulsars en
dc.subject Stellar Evolution en
dc.subject Supernova Remnants en
dc.subject Vectors (Mathematics) en
dc.subject Velocity Distribution en
dc.subject Angular Distribution en
dc.subject Binary Stars en
dc.subject Neutron Stars en
dc.subject Spatial Distribution en
dc.subject Orbital Velocity en
dc.title On the orientation of the pulsar space velocity vector relative to the spin axis en
dc.type Article en


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