Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T15:11:10.848Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsar Observations at Molonglo

Published online by Cambridge University Press:  25 April 2016

A. E. Vaughan  and
M. I. Large
A. E. Vaughan
Affiliation:
Cornell-Sydney University Astronomy Centre School of Physics, University of Sydney
M. I. Large
Affiliation:
Cornell-Sydney University Astronomy Centre School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

The physical properties and spatial distribution of 12 pulsars discovered with the Molonglo radio telescope have been discussed by Mills. Several more pulsars have been detected and details will be published when the measurements are complete. Parameters of a recently discovered pulsar, MP 0628, are given in Table I. All the Molonglo pulsars have been found by visual examination of chart records. The use of pulse lengthening circuits to improve the visibility of pulsars on slow charts, and the continuation of the observations over several hundred hours with the greatest available sensitivity have been factors contributing significantly to the success of the Molonglo pulsar search.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 220 - 223
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Mills, B. Y., Proc. ASA, 1, 176 (1969).Google Scholar
2 Large, M. I., Vaughan, A. E. and Wielebinski, R., Nature, 220, 753 (1968).CrossRefGoogle Scholar