Meikle, W. P. S. and Drever, R. W. P. and Haynes, R. F. and Shakeshaft, J. R. and Charman, W. N. and Jelley, J. V. (1972) A Search for Isolated Radio Pulses from the Crab Nebula at 151.5 MHz. Monthly Notices of the Royal Astronomical Society, 160 (1). 5P-8P. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20160119-072042286
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Abstract
A search has been made for large bursts of radio emission at 151.5 MHz from the direction of the Crab Nebula. In 605 hr of observation, no events exceeding a flux of 1.4 × 10^(−22) W m^(−2) Hz^(−1) were detected. This therefore sets an upper limit for the energy in radio pulses from the direction of the Crab Nebula which might be associated with the events recorded in the gravitational wave experiments of Weber. Implications of the results with regard to ‘strong pulses’ and phase fluctuations in the periodic emissions from the pulsar NP 0532 are also examined.
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| Additional Information: | © 1972 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1972 August 21. First published online March 1, 1972. We wish to thank Mr A. McKellar and Mr J. H. Fruin for valuable technical assistance with the equipment at Glasgow and Harwell respectively. | ||||||||||||
| Record Number: | CaltechAUTHORS:20160119-072042286 | ||||||||||||
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20160119-072042286 | ||||||||||||
| Official Citation: | W. P. S. Meikle, R. W. P. Drever, R. F. Haynes, J. R. Shakeshaft, W. N. Charman, and J. V. Jelley A Search for Isolated Radio Pulses from the Crab Nebula at 151.5 MHz MNRAS (1972) Vol. 160 5P-8P doi:10.1093/mnras/160.1.5P First published online March 1, 1972 | ||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||
| ID Code: | 63737 | ||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||
| Deposited By: | Ruth Sustaita | ||||||||||||
| Deposited On: | 21 Jan 2016 20:31 | ||||||||||||
| Last Modified: | 21 Jan 2016 20:31 |
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