Citation
Palmer, David M. (1992) Gamma-ray imaging observations of Supernova 1987A. Dissertation (Ph.D.), California Institute of Technology. http://resolver.caltech.edu/CaltechTHESIS:09012011-153518265
Abstract
The Caltech imaging γ-ray telescope has made four balloon flights from Alice Springs, Australia, to observe the hard X-ray and γ-ray emission from Supernova 1987 A as it evolved between 1987 May and 1989 April. We have detected γ-rays with the time behavior and spectral signature expected from freshly-synthesized radioisotopes embedded in a cloud of ejecta. In particular, we detect the 847 and 1238 keY γ-ray lines produced by the decay of ^(56)Co, and the continuum spectrum expected from Compton scattering of these γ-trays. The results of these observations are compared with other measurements and with theoretical models of supernovae, and it is found that our results are consistent with core-collapse models for SN 1987A in which the centrally-produced radioisotopes have propagated outwards to mix with the ejecta.
| Item Type: | Thesis (Dissertation (Ph.D.)) |
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| Subject Keywords: | Physics |
| Degree Grantor: | California Institute of Technology |
| Division: | Physics, Mathematics and Astronomy |
| Major Option: | Physics |
| Thesis Availability: | Restricted to Caltech community only |
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| Thesis Committee: |
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| Defense Date: | 28 February 1992 |
| Record Number: | CaltechTHESIS:09012011-153518265 |
| Persistent URL: | http://resolver.caltech.edu/CaltechTHESIS:09012011-153518265 |
| Default Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
| ID Code: | 6645 |
| Collection: | CaltechTHESIS |
| Deposited By: | Tony Diaz |
| Deposited On: | 07 Sep 2011 18:28 |
| Last Modified: | 26 Dec 2012 04:38 |
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