Published February 1988
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Journal Article
Open
A search for infrared pulsations from PSR 1951 + 32
Chicago
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Abstract
Observations have been conducted on the recently discovered short period pulsar PSR 1951+32 in the radio nebula CTB 80 in an attempt to detect pulsed infrared emission. A strong upper limit is placed on any pulsed, infrared component below that expected from a formally proposed optical candidate for the pulsar. This limit is consistent with proposed scaling laws for high-energy emission.
Additional Information
© 1988 European Southern Observatory. Received November 24, accepted November 26, 1987.Attached Files
Published - 1988A+A___191L___7C.pdf
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1988A+A___191L___7C.pdf
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- Eprint ID
- 74647
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- CaltechAUTHORS:20170301-132014168
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2017-03-01Created from EPrint's datestamp field
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2019-10-03Created from EPrint's last_modified field
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- Division of Geological and Planetary Sciences (GPS)