Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-03T00:47:52.396Z Has data issue: false hasContentIssue false
  • English
  • Français

Three New Pulsars Near Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

D. K. Mohanty
D. K. Mohanty*
Affiliation:
Radio Astronomy Centre(TIFR), Ootacamund, India

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A search for pulsars in the directions of twenty Galactic supernova remnants (SNRs) was carried out at 327 MHz with the Ooty Radio Telescope (ORT). We have measured the P for one of the pulsars which is just outside the shell of SNR W44 and discuss here the possibility of its association with the HI shell around W44. The parameters of the remaining two pulsars have not yet been determined with sufficient accuracy to suggest association with the respective SNRs.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 503 - 504
Copyright
Copyright © Reidel 1983 

References

Manchester, R.N. and Taylor, J.N., 1977, Pulsars, Freeman Co.Google Scholar
Knapp, G.R. and Kerr, F.J., 1974, Astron. Astrophys., 33, 463.Google Scholar
Stacy, J.G. and Jackson, P.D., 1982, Nature, 296, 42.Google Scholar