Can Ejecta‐dominated Supernova Remnants be Typed from Their X‐Ray Spectra? The Case of G337.2−0.7-Reference-Cited by-同舟云学术

Can Ejecta‐dominated Supernova Remnants be Typed from Their X‐Ray Spectra? The Case of G337.2−0.7

Published:2006-08 Issue:2 Volume:646 Page:982-1000
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Rakowski Cara E.,Badenes Carles,Gaensler B. M.,Gelfand Joseph D.,Hughes John P.,Slane Patrick O.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference72 articles.

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2. Abundances of the elements: Meteoritic and solar

3. Arnaud, K. A. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & J. Barnes (San Francisco: ASP), 17

4. Badenes, C. 2004, Ph.D. thesis, Univ. Politecnica de Catalunya

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

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