Pulsars - Space kinematic characteristics and their connection with supernova remnants

Details Pulsars - Space kinematic characteristics and their connection with supernova remnants Pulsars - Space kinematic characteristics and their connection with supernova remnants

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115....1a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 1, Oct. 1985, p. 1-29.

Astronomy and Astrophysics

Astrophysics

4

Pulsars, Star Distribution, Supernova Remnants, Kinematics, Milky Way Galaxy, Radial Distribution, Stellar Evolution, X Ray Sources

Scientific paper

The galactic distribution of pulsars and shell remnants of supernovas is investigated on the basis of newly estimated parameters. Attention was paid to accounting for all possible selection effects, and an attempt was made to reveal a statistically pure ensemble of objects so as to study the radial and z-distribution of pulsars and supernova remnants (SNRs). The radial distribution of pulsars is found to be annular with maximum pulsar surface density at distances of about 5.3 kpc (assuming the sun to be 8.5 kpc from the galactic center). Massive runaway OB-stars and type-I supernovas are also discussed.

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