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Galactic distribution of pulsarsThe density distributions of pulsars in luminosity, period, Z-distance, and galactocentric distance were derived using a uniform sample of pulsars detected during a 408 MHz pulsar survey at Jodrell Bank. There are indications of a fine scale structure in the spatial distribution and evidence that there is a general correlation with other galactic populations and the overall spiral structure. The electron layer in the galaxy is shown to be wider than the pulsar layer and uniform on a large scale. The number of pulsars in the galaxy was estimated and used to derive the pulsar birthrate.
Document ID
19760022041
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Seiradakis, J. H.
(Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Date Acquired
August 8, 2013
Publication Date
June 1, 1976
Publication Information
Publication: NASA. Goddard Space Flight Center The Struct. and Content of the Galaxy and Galactic Gamma Rays
Subject Category
Astronomy
Accession Number
76N29129
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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