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- W93081722 abstract "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." @default.
- W93081722 created "2016-06-24" @default.
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- W93081722 date "2004-12-01" @default.
- W93081722 modified "2023-09-27" @default.
- W93081722 title "Candidates for pulsar/supernova remnant associations" @default.
- W93081722 hasPublicationYear "2004" @default.
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