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The deepest search yet for pulsed emission from the supernova remnant Cassiopeia A shows there to be no clear pulsar candidate at 408 MHz with a mean flux density over 80 mJy and period between 0.02 and 4 s. A similar search at 81.5 MHz places an upper limit of 700 mJy for periods between 1 and 4 s.
|Glasgow Author(s):||Woan, Prof Graham|
|Authors:||Woan, G., and Duffett-Smith, P.G.|
|College/School:||College of Science and Engineering > School of Physics and Astronomy|
|Journal Name:||Monthly Notices of the Royal Astronomical Society|
|Publisher:||Wiley-Blackwell Publishing Ltd.|