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Exosat Observations of Young SNRs

Published online by Cambridge University Press:  12 April 2016

A. Smith
A. Smith*
Affiliation:
Space Science Department of ESA, ESTEC, NOORDWIJK, The Netherlands

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In this work we study the 2 – 10 keV spectra of eight relatively well known SNRs. These spectra were obtained with the medium energy experiment on-board the X-ray satellite EXOSAT. Details of the EXOSAT mission can be found in Taylor et al 1981 and the ME experiment is described in Turner, Smith and Zimmerman 1981. The ME experiment is well suited for this study since it provides a high sensitivity and a narrow field of view (45 ' FWHM). These spectra are considered in the context of a model in which the 2–10 keV continuum arises from shock heated interstellar material.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 119 - 124
Copyright
Copyright © Cambridge University Press 1988

References

Braun, R., 1985, Thesis, Sterrewacht, Leiden, Netherlands.Google Scholar
Caswell, J.L., Clark, D.H., and Crawford, D.F., Austr, J. Phys. Suppl., 37, 39.Google Scholar
Claas, J. et al 1987, in preparation.Google Scholar
Hamilton, A.J.S., Sarazin, C.L. and Chevalier, R.A. 1983, Ap. J. Suppl., 51, 115.Google Scholar
Ilovaisky, S.A., and Lequeux, J., 1972, Astr. Astro. 18, 169.Google Scholar
Jansen, F., Smith, A., Bleeker, J.A.M., deKorte, P.A.J., Peacock, A. and White, N.E., 1987 submitted to Ap.J.Google Scholar
Jones, L.R., Pye, J.P. and Culhane, J.L. Proc. Int. Symp. on X-ray Astronomy, Bologna, 1984, p321.Google Scholar
Peacock, A., Smith, A., de Vries, J., Jansen, F., de Korte, P.A.J. and Bleeker, J.A.M., 1987, in preparation.Google Scholar
Peacock, A. and Smith A. in preparation.Google Scholar
Pye, J.P., Pounds, K.A., Rolf, D.P. Seward, F.D., Smith, A. and Willingale, R., M.N.R.A.S., 194, 569, 1981.Google Scholar
Slee, O.B., and Duik, G.A., 1974, Galactic Radio Astronomy, ed. Kerr, F.K. and Simonson, S.C. III, Reidel press p 347 Google Scholar
Smith, A., Jones, L.R., Peacock, A., and Pye, J.P. Ap. J. 296, 469, 1985.Google Scholar
Smith, A. Davelaar, J. Peacock, A. Taylor, B.G., Morini, M. nd Robba, N.R., 1987a, submitted to Ap.J.Google Scholar
Smith, A. Peacock, A. Arnaud, M. Ballet, J., Rothenflug, R. and Rocchia, R. 1987b, in preparation.Google Scholar
Taylor, B.G., Andresen, R.D., Peacock, A. and Zobl, R., 1981, Space Sci. Rev., 54, 229.Google Scholar
Turner, M.J.L., Smith, A. and Zimmerman, H.U., 1981, Space Sci. Rev., 30, 513.Google Scholar
Wilson, T.L. 1970, Ap J. Letts. 7, 95.Google Scholar