Palumbo, G. G. C. and Mandolesi, N. and Morigi, G. and Baird, G. A. and Delaney, T. and Meikle, W. P. S. and Drever, R. W. P. and Jelley, J. V. and Fruin, J. H. and Partridge, R. B. (1978) Upper limits for the microwave pulsed emission from supernova explosions in clusters of galaxies. Astrophysics and Space Science, 54 (2). pp. 355-363. ISSN 0004-640X. doi:10.1007/BF00639440. https://resolver.caltech.edu/CaltechAUTHORS:20151224-092000963
Full text is not posted in this repository. Consult Related URLs below.
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20151224-092000963
Abstract
Between 1972 and 1975 an international collaborative search was carried out for prompt 10 GHz emission at the onset of supernovae. The motivations and techniques involved in this effort are described, and the results of the three years' work are summarized. No pulses from supernovae were detected, the best upper limit being 4×10^(43) ergs in a 40 MHz band at 10 GHz for a pulse time-scale ≲0.5 s. Methods for improving this limit are briefly described.
| Item Type: | Article | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Related URLs: |
| |||||||||
| Additional Information: | © 1978 by D. Reidel Publishing Company, Dordrecht-Holland. Received 4 October, 1977. Jn an experiment which lasted over three years, and in which five groups in different countries were engaged, it is not surprising that many people have contributed in various ways at different stages of development. We wish to express here our gratitude to all of them. In particular, thanks are due to: S. Colgate for illuminating and stimulating discussion and for expanding, adopting and unravelling his theory for our benefit; G. Cavallo for criticisms and discussions at various stages of this work and comments on the manuscripts; and C. T. Kowal for kindly providing the available information about the SNe in Perseus. Part of the arguments and data included in this paper were presented by some of us at the Erice Summer School on Fast Transient Phenomena (Erice, 28 June-7 July, 1976). The Harwell and Bologna groups wish to acknowledge NATO for financial support, under Research Grant No. 653. | |||||||||
| Funders: |
| |||||||||
| Issue or Number: | 2 | |||||||||
| DOI: | 10.1007/BF00639440 | |||||||||
| Record Number: | CaltechAUTHORS:20151224-092000963 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20151224-092000963 | |||||||||
| Official Citation: | Upper limits for the microwave pulsed emission from supernova explosions in clusters of galaxies G. G. C. Palumbo, N. Mandolesi, G. Morigi, G. A. Baird, T. Delaney, W. P. S. Meikle, R. W. P. Drever, J. V. Jelley, J. H. Fruin... Astrophysics and Space Science April 1978, Volume 54, Issue 2, pp 355-363 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 63221 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Ruth Sustaita | |||||||||
| Deposited On: | 24 Dec 2015 17:28 | |||||||||
| Last Modified: | 10 Nov 2021 23:13 |
Repository Staff Only: item control page
