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New Observations of HI Absorption for Pulsars
Published online by Cambridge University Press: 14 August 2015
Extract
The second Molongo pulsar survey (Manchester et al., 1978) provides a large sample of pulsars in the southern sky. It is of interest to obtain non-dispersion-dependent distances for as many of these pulsars as possible. Since most of these pulsars are relatively weak, a system of high sensitivity is required. In this paper we report on preliminary observations made at Parkes during June 1980 with such a system.
- Type
- X. Galactic Distribution of Pulsars
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- Copyright © Reidel 1981
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