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Discovery of X-Ray Emission from the Radio SNR G352.7-0.1

Published online by Cambridge University Press:  25 May 2016

K. Kinugasa ,
K. Torii ,
H. Tsunemi ,
S. Yamauchi ,
K. Koyama  and
T. Dotani
K. Kinugasa
Affiliation:
Graduate School of Science, Osaka University 1-1 Machikaneyama-cho, Toyonaka, Osaka 560, Japan
K. Torii
Affiliation:
Graduate School of Science, Osaka University 1-1 Machikaneyama-cho, Toyonaka, Osaka 560, Japan
H. Tsunemi
Affiliation:
Graduate School of Science, Osaka University 1-1 Machikaneyama-cho, Toyonaka, Osaka 560, Japan
S. Yamauchi
Affiliation:
Faculty of Humanities and Social Sciences, Iwate University
K. Koyama
Affiliation:
Graduate School of Science, Kyoto University
T. Dotani
Affiliation:
Institute of Space and Astronautical Science

Extract

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One major objective of our ASCA Galactic Plane Survey Project (AGPSP) is, utilizing the wide and high energy band (up to 10 keV) X-ray imaging capability and the high spectral resolving power of ASCA, to search possible X-ray SNRs in the Galactic inner disk. The observation of the field including G352.7-0.1 reported in this paper, was performed on 1996 March 14 during the first AO4 survey. We report on the X-ray SNR G352.7-0.1 found in AGPSP. G352.7-0.1 is one of the radio SNRs (Green 1996), and is classified as a shell-like SNR with the size of 8' x 6'.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 251 - 252
Copyright
Copyright © Kluwer 1998