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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S331(12), p. 213-215, 2017

DOI: 10.1017/s1743921317004835

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Searching for Young Type Ia Supernova Remnants in M83

Journal article published in 2017 by Chuan-Jui Li ORCID, You-Hua Chu ORCID, Po-Sheng Ou
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractYoung Type Ia supernova remnants (SNRs) are characterized by Balmer-dominated optical spectra, well-defined shell morphologies, > 1036 ergs s−1 X-ray luminosities, and a lack of massive stars and dense interstellar gas in their vicinity. Applying these characteristics and using archival deep HST and Chandra observations of M83, we search for young Type Ia SNRs in this spiral galaxy. This is a very difficult task!

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