Discriminating the progenitor type of supernova remnants with Iron K-shell emission

Discriminating the progenitor type of supernova remnants with Iron K-shell emission

Supernova remnants (SNRs) retain crucial information about both their parent explosion and circumstellar material left behind by their progenitor. However, the complexity of the interaction between supernova ejecta and ambient medium often blurs this information, and it is not uncommon for the basic...

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Main Authors: Yamaguchi, Hiroya (Author), Badenes, Carles (Author), Petre, Robert (Author), Nakano, Toshio (Author), Castro, Daniel (Contributor), Enoto, Teruaki (Author), Hiraga, Junko S. (Author), Hughes, John P. (Author), Maeda, Yoshitomo (Author), Nobukawa, Masayoshi (Author), Safi-Harb, Samar (Author), Slane, Patrick O. (Author), Smith, Randall K. (Author), Uchida, Hiroyuki (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-01-12T19:15:55Z.
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