Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95..308a&link_type=abstract
Astronomy and Astrophysics, vol. 95, no. 2, Mar. 1981, p. 308-315.
Astronomy and Astrophysics
Astrophysics
12
Galactic Structure, Pulsars, Star Distribution, Stellar Evolution, Galactic Rotation, Neutron Stars, Spatial Distribution, Statistical Analysis, Stellar Luminosity
Scientific paper
It is shown that a lack of knowledge concerning interstellar electron density, the true spatial distribution of pulsars, the radio luminosity source distribution of pulsars, the real ages and real aging rates of pulsars, the beaming factor (and other unknown factors causing the known sample of about 350 pulsars to be incomplete to an unknown degree) is sufficient to cause a minimum uncertainty of a factor of 20 in any attempt to determine pulsar birth or death rates in the Galaxy. It is suggested that this uncertainty must impact on suggestions that the pulsar rates can be used to constrain possible scenarios for neutron star formation and stellar evolution in general.
Arnett David. W.
Lerche Ian
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