Candidates for pulsar/supernova remnant associations

Details Candidates for pulsar/supernova remnant associations Candidates for pulsar/supernova remnant associations

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004pabei..22..308t&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 22, No. 4, p. 308 - 317 (2004)

Astronomy and Astrophysics

Astrophysics

4

Astrophysics, Associations, Review, Pulsar, Supernova Remnant, Statistics

Scientific paper

We list a sample of 50 pairs of pulsar (PSR) and supernova remnant (SNR) associations which have been suggested from over 230 SNRs and 1300 PSRs. At least 20 pairs of them are real because the pulsar wind nebulae around the PSRs have been detected. We analyze factors which may result in the deficit of associations. Considering recent observational progress, we simply discuss reality of the 50 pairs cataloged associations and the possibility to detect more PSR/SNR associations. We give a detailed discussion aimed at three pairs of likely PSR/SNR associations PSR J1811-1925/SNR G11.2-0.3, PSR J1932+2020/SNR G55.0+0.3 and PSR J1706/SNR G343.1-2.3 in our sample.

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