Suzaku X-ray observations of the mixed-morphology supernova remnant CTB 1-Reference-Cited by-同舟云学术

Suzaku X-ray observations of the mixed-morphology supernova remnant CTB 1

Published:2018-10-31 Issue:6 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Katsuragawa Miho¹²,Nakashima Shinya³,Matsumura Hideaki²,Tanaka Takaaki⁴,Uchida Hiroyuki⁴,Lee Shiu-Hang⁵,Uchiyama Yasunobu⁶,Arakawa Masanori⁶⁷,Takahashi Tadayuki¹²

Affiliation:

1. Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

2. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan

3. RIKEN High Energy Astrophysics Laboratory, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan

4. Department of Physics, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, Kyoto 606-8502, Japan

5. Department of Astronomy, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, Kyoto 606-8502, Japan

6. Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo 171-8501, Japan

7. Astrophysical Big Bang Laboratory, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan

Funder

Japan Society for the Promotion of Science

RIKEN

Kyoto University Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/6/110/27072141/psy114.pdf

Reference49 articles.

1. THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG

2. Abundances of the elements: Meteoritic and solar

3. X-RAY EVOLUTION OF PULSAR WIND NEBULAE

4. Modeling W44 as a Supernova Remnant in a Density Gradient with a Partially Formed Dense Shell and Thermal Conduction in the Hot Interior. I. The Analytical Model

5. ROSATObservations of the Supernova Remnant CTB 1

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