Hopkins, Philip F. (2017) Supernovae, supercomputers, and galactic evolution. Physics Today, 70 (4). pp. 70-71. ISSN 00319228. doi:10.1063/PT.3.3533. https://resolver.caltech.edu/CaltechAUTHORS:20170518-133304820
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Abstract
The stars in a galaxy emit radiation and solar winds, and they sometimes die in fantastic explosions. Supercomputer simulations are now beginning to assess how those energy releases affect the galaxy’s life.
| Item Type: | Article | |||||||||
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| Additional Information: | © 2017 American Institute of Physics. | |||||||||
| Group: | Astronomy Department | |||||||||
| Issue or Number: | 4 | |||||||||
| DOI: | 10.1063/PT.3.3533 | |||||||||
| Record Number: | CaltechAUTHORS:20170518-133304820 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170518-133304820 | |||||||||
| Official Citation: | Supernovae, supercomputers, and galactic evolution Philip F. Hopkins Physics Today 70, 70 (2017); http://doi.org/10.1063/PT.3.3533 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 77584 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Ruth Sustaita | |||||||||
| Deposited On: | 18 May 2017 21:07 | |||||||||
| Last Modified: | 15 Nov 2021 17:32 |
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