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The X-Ray Spectrum of the Cygnus Loop with GSPC

Published online by Cambridge University Press:  12 April 2016

Hiroshi Tsunemi ,
Makoto Manabe  and
Koujun Yamashita
Hiroshi Tsunemi
Affiliation:
Department of Physics, Faculty of Science, Osaka University, 1-1, Machikaneyama-cho, Toyonaka, Osaka 560Japan
Makoto Manabe
Affiliation:
Department of Physics, Faculty of Science, Osaka University, 1-1, Machikaneyama-cho, Toyonaka, Osaka 560Japan
Koujun Yamashita
Affiliation:
Department of Physics, Faculty of Science, Osaka University, 1-1, Machikaneyama-cho, Toyonaka, Osaka 560Japan

Extract

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We observed the Cygnus Loop with Gas Scintillation Proportional Counter (GSPC) on board Tenma satellite. GSPC has an energy resolution two times better than that of a proportional counter (PC). Fig. 1 shows the spectrum with the crosses being the pulse height data with ± 1σ statistics. Superposed upon the data point is the best fit model spectra folded through the detector response.

Type
Part III. Chemical and Dynamical Structures of Exploding Stars
Information
International Astronomical Union Colloquium , Volume 108: Atmospherics Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion , 1988 , pp. 456 - 457
Copyright
Copyright © Springer-Verlag 1988

References

Allen, C.W. 1973, Astrophysical Quantities.Google Scholar
Charles, P.A., Kahn, S.M., and McKee, C.F. 1985, Ap. J., 295 456.Google Scholar
Gorenstein, P., et al. 1971. Science, 172 369.Google Scholar
Inoue, H., et al. 1979, X-ray Astronomy, (Oxford, Pergamon Press.) 309.Google Scholar
Raymond, J.C., and Smith, B.W., 1977 Ap. J., suppl., 35 419.Google Scholar
Vedder, P.W., et al. 1986, Ap. J., 307 269.CrossRefGoogle Scholar