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New Observations of HI Absorption for Pulsars

Published online by Cambridge University Press:  14 August 2015

R. N. Manchester ,
K. J. Wellington  and
P.M. McCulloch
R. N. Manchester
Affiliation:
CSIRO, Division of Radiophysics, Sydney, Australia
K. J. Wellington
Affiliation:
CSIRO, Division of Radiophysics, Sydney, Australia
P.M. McCulloch
Affiliation:
University of Tasmania, Hobart, Australia

Extract

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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
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 445 - 448
Copyright
Copyright © Reidel 1981 

References

Ables, J.G. and Manchester, R.N.: 1976, Astron. Astrophys., 50, p. 177.Google Scholar
Manchester, R.N., Lyne, A.G., Taylor, J.H., Durdin, J.M., Large, M.I. and Little, A.G.: 1978, Mon. Not. R. Astron. Soc, 185, p. 409.Google Scholar
Weisberg, J.M., Boriakoff, V. and Rankin, J.: 1979, Astron. Astrophys., 77, p. 204.Google Scholar
Weisberg, J.M., Rankin, J., and Boriakoff, V.: 1980, Astron. Astrophys., 88, p. 94.Google Scholar