Please use this identifier to cite or link to this item:
Title: On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52
Authors: Srinivasan, G.
Dwarakanath, K.S.
Radhakrishnan, V.
Issue Date: 20-Jun-1982
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.
ISSN: 0011-3891
Copyright: Indian Academy of Sciences, Bangalore, India.
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1982 CS V51 p596.pdf4p.281.83 kBAdobe PDFView/Open

Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.