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A Shell SNR Associated with PSR1930+22?
Published online by Cambridge University Press: 12 April 2016
Abstract
Observations at 408 and 1420 MHz are reported which show a large (1.7 degree diameter) faint shell of nonthermal emission partially surrounding PSR1930+22. This may be the SNR associated with the pulsar, whose spin-down age is only 40000 years.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 339 - 342
- Copyright
- Copyright © Cambridge University Press 1988
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