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Features in the Soft X-ray Background

Published online by Cambridge University Press:  12 April 2016

R. Rothenflug
R. Rothenflug*
Affiliation:
Service d’Astrophysique (DPHG/IRF)C.E.N. Saclay(France)

Abstract

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The soft X-ray background is explained in terms of emission coming from hot gas. Most of these soft X-ray data were obtained by proportional counters with a poor energy resolution. Instruments having the capability to resolve lines were only flown by two groups: a GSPC by a Japanese group and a SSD by a french-american collaboration. They both detected the 0 VII line emission coming from the soft X-ray background and so proved the thermal nature of the emission. The implications of these results on possible models for the local hot medium will be discussed. The same detectors observed part of the North Polar Spur. They detected emission lines coming from different species (0 VII,Fe XVII,Ne IX). Spatial variations of line ratios for this object could be due to non-equilibrium ionization effects.

Type
4. Supernova Remnants, Soft X-ray Background
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 146 - 155
Copyright
Copyright © Cambridge University Press 1990

References

Arnaud, M., Rothenflug, R., Rocchia, R., 1984, Physica Scripta, Vol. T7, p. 48 Google Scholar
Arnaud, M., Rothenflug, R., 1985, Astron. Astrop. Suppl. Ser. 60, 425 Google Scholar
Arnaud, M., Rothenflug, R., 1986, Adv.Space Res., Vol. 6, No. 2, p119 Google Scholar
Arnaud, M., Rothenflug, R., 1989, in preparationGoogle Scholar
Berkuijsen, E.M., 1973, Astr.,Ap., 24, 143 Google Scholar
Bloch, J.J., Jahoda, K., Juda, M., McCammon, D.,D.N., Sanders, W.T., Snowden, S.L. 1986, Ap.J.(Letters) 308, L59 Google Scholar
Bloch, J.J., Priedhorsky, W.C., Smith, B.W., 1988, these proceedingsGoogle Scholar
Bruhweiler, F.C., Gull, T.R., Kafatos, M., Sofia, S., 1980, Ap.J.(Letters) 238, L27 Google Scholar
Cox, D.P., Anderson, P.R., 1982, Ap.J. 253, 268 Google Scholar
Cox, D.P., Reynolds, R.J., 1987, Ann. Rev. Astron. Astrophys., Vol. 25, 303 Google Scholar
Davelaar, J., Bleeker, J.A.M., Deerenberg, A.J.M., 1980, Astr.,Ap., 92, 231 Google Scholar
Heiles, C., Chu, Y.H., Reynolds, R.J., Yegingil, I., Troland, T.H., 1980, Ap.J., 242, 533 Google Scholar
Inoue, H., Koyama, K., Matsuoka, M., Ohashi, T., Tanaka, Y., Tsunemi, H., 1979, Ap.J., 227, L65 1980, Ap.J., 238, 886 Google Scholar
Iwan, D.A., 1980, Ap.J. 239, 316 Google Scholar
Kato, T., 1976, Ap.J.Sup. 30, 397 Google Scholar
McCammon, D., Burrows, D.N., Sanders, W.T., Kraushaar, W.L., 1983, Ap.J., 269, 107 Google Scholar
Marshall, F. J., Clark, G.W., 1984, Ap.J. 287, 633 Google Scholar
Masai, K., 1984, Astrophysics and Space science, 98, 367 Google Scholar
Mewe, R., Gronenschild, E.H.B.M., Van den Oord, G.H.J., 1985, Astron. Astrop. Sup. Ser., 62, 197 Google Scholar
Mewe, R., Lemen, J.R., Van den Oord, G.H.J., 1986, Astron. Astrop. Sup. Ser., 65, 511 Google Scholar
Meyer, J.P., 1985, Ap.J.Suppl.Ser., 57, 151 Google Scholar
Nousek, J.A., Cowie, L.L., Hu, E., Linblad, C.J., Garmire, G.P., 1981, Ap.J., 248, 152 Google Scholar
Nousek, J.A., Fried, P.M., Sanders, W.T., Kraushaar, W.L., 1982, Ap.J. 258, 83 CrossRefGoogle Scholar
Rocchia, R., Arnaud, M., Blondel, C., Cheron, C., Christy, J.C., Rothenflug, R., Schnopper, H.W., Delvaille, J.P., 1984, Astron. Astrop. 130, 53 Google Scholar
Rothenflug, R., Arnaud, M., Blondel, C., Rocchia, R., 1984, Physica Scripta, Vol. T7 p. 62 Google Scholar