DISCRIMINATING THE PROGENITOR TYPE OF SUPERNOVA REMNANTS WITH IRON K-SHELL EMISSION-Reference-Cited by-同舟云学术

DISCRIMINATING THE PROGENITOR TYPE OF SUPERNOVA REMNANTS WITH IRON K-SHELL EMISSION

Published:2014-04-03 Issue:2 Volume:785 Page:L27
ISSN:2041-8205
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Yamaguchi Hiroya^ORCID,Badenes Carles,Petre Robert^ORCID,Nakano Toshio,Castro Daniel,Enoto Teruaki^ORCID,Hiraga Junko S.,Hughes John P.,Maeda Yoshitomo,Nobukawa Masayoshi,Safi-Harb Samar,Slane Patrick O.,Smith Randall K.^ORCID,Uchida Hiroyuki

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/2041-8205/785/2/L27/pdf

Reference51 articles.

1. Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants. II. Parameters Affecting the Spectrum

2. Constraints on the Physics of Type Ia Supernovae from the X‐Ray Spectrum of the Tycho Supernova Remnant

3. Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification

4. Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?

5. X-Ray-Emitting Ejecta of Supernova Remnant N132D

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