Constraining magnetic field amplification in SN shocks using radio observations of SNe 2011fe and 20...
Constraining magnetic field amplification in SN shocks using radio observations of SNe 2011fe and 2014J
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We modeled the radio non-detection of two Type Ia supernovae (SNe) 2011fe and 2014J considering synchrotron emission from the interaction between SN ejecta and the circumstellar medium. For an ejecta with the outer part having a power law density structure we compare synchrotron emission with radio observations. Assuming that 20\(\%\) of the bulk s...
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Constraining magnetic field amplification in SN shocks using radio observations of SNe 2011fe and 2014J
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TN_cdi_proquest_journals_2075995334
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2075995334
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1705.04204
