Article contents
Supernova Remnant CTB 80 and PSR 1951+32
Published online by Cambridge University Press: 12 April 2016
Abstract
The 39.5 ms pulsar PSR 1951+32 and the remnant with which it is associated, CTB 80, have both been observed with the recently upgraded Westerbork synthesis array (WSRT). Parts of CTB 80 have been observed over the frequency coverage from 0.3 to 8 GHz, while PSR 1951+32 has been observed from 0.3 to 1.6 GHz. The results are described and discussed in the context of the pulsar-remnant association.
- Type
- Part 7. The Surrounding of Pulsars
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 509 - 512
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
- 1
- Cited by