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Supernovae, supercomputers, and galactic evolution

Hopkins, Philip F. (2017) Supernovae, supercomputers, and galactic evolution. Physics Today, 70 (4). pp. 70-71. ISSN 00319228. 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
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1063/PT.3.3533DOIArticle
http://physicstoday.scitation.org/doi/full/10.1063/PT.3.3533PublisherArticle
ORCID:
AuthorORCID
Hopkins, Philip F.0000-0003-3729-1684
Additional Information:© 2017 American Institute of Physics.
Group:Astronomy Department
Issue or Number:4
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:03 Oct 2019 17:59

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