Multifrequency study of a new Fe-rich supernova remnant in the Large Magellanic Cloud, MCSNR J0508−6902-Reference-Cited by-同舟云学术

Multifrequency study of a new Fe-rich supernova remnant in the Large Magellanic Cloud, MCSNR J0508−6902

Published:2014-02-05 Issue:1 Volume:439 Page:1110-1124
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bozzetto L. M.,Kavanagh P. J.,Maggi P.,Filipović M. D.,Stupar M.,Parker Q. A.,Reid W. A.,Sasaki M.,Haberl F.,Urošević D.,Dickel J.,Sturm R.,Williams R.,Ehle M.,Gruendl R.,Chu Y.-H.,Points S.,Crawford E. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/439/1/1110/9502114/stu051.pdf

Reference113 articles.

1. MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS

2. Evidence of short-lived SN Ia progenitors

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

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

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