The origin of recombining plasma and the detection of the Fe-K line in the supernova remnant W 28
Author:
Affiliation:
1. Department of Physics, Faculty of Science, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, Kyoto 606-8502, Japan
Funder
MEXT
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/70/3/35/25055017/psy022.pdf
Reference49 articles.
1. FERMILARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT W28 (G6.4–0.1)
2. Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field
3. Abundances of the elements: Meteoritic and solar
4. Shocked Molecular Gas Associated with the Supernova Remnant W28
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