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|Title:||On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52|
|Publisher:||Indian Academy of Sciences, Bangalore, India.|
|Citation:||Current Science, 1982, Vol. 51, p596-599.|
|Abstract:||Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators.|
|Copyright:||Indian Academy of Sciences, Bangalore, India.|
|Appears in Collections:||Research Papers (A&A)|
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