Hostname: page-component-77c89778f8-gq7q9 Total loading time: 0 Render date: 2024-07-18T22:30:45.310Z Has data issue: false hasContentIssue false
  • English
  • Français

2. X-Ray Astronomy

Published online by Cambridge University Press:  24 November 2021

K.A. Pounds

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

X-ray astronomy has continued to flourish in the three years covered by the present report (to June 1987) despite the continuing scarcity of new missions. The European EXOSAT has probably made the greatest impact during this period, carrying out over 2000 separate observations up to it’s loss of attitude control in April 1986. A major reason for the success of EXOSAT was the unusual spacecraft orbit which provided uniquely long source exposures, uninterrupted by Earth occultation, of up to 70 hours duration. The continuous light curves of many galactic and extragalactic sources have proved particularly valuable in studying details of time variability over a broad frequency range and in this respect the EXOSAT data archive is unlikely to be superceded in this century. For several months after the demise of EXOSAT, astronomers had no operational X-ray satellite for the first time since the launch of Uhuru in 1970. This unfortunate state of affairs ended in February 1987 with the successful launch of the Japanese ASTRO-C satellite. Three months later, observations began with several X-ray instruments on board the Soviet MIR space station and at the time of writing both GINGA (the post-launch name of ASTRO-C) and the MIR instruments are working well.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 1 , 1988 , pp. 602 - 607
Copyright
Copyright © Kluwer 1988 

References

Arnaud, K.A. et al: 1985, Mon. Not. R. astr. Soc. 217, p. 105.CrossRefGoogle Scholar
Barstow, M.A., Holberg, J.B., Grauer, A.D. and Winget, D.E.: 1986, Ap. J., 306, L25.CrossRefGoogle Scholar
Barstow, M.A.: 1987, Proceedings of the Nato AS1 “Hot Thin Plasmas in Astrophysics, in press.Google Scholar
Boldt, E.: 1987, Phys. Rep. 146, p. 216.CrossRefGoogle Scholar
Charles, P.A., Jones, D.C. and Naylor, T.: 1986, Nature, 323, p. 417.CrossRefGoogle Scholar
Edge, A.C., Stewart, G.C. and Smith, A.: 1987, NRAO Workshop, 16, p. 105.Google Scholar
Edge, A.C., Stewart, G.C. and McHardy, I.M.: 1988, Proc. NATO Adv. St. Inst., Cargese.Google Scholar
Fabbiano, G. and Trinchieri, G.: 1985, Astrophys. J., 296, p. 430.CrossRefGoogle Scholar
Fabian, A.C. et al: 1985, Mon. Not. R. astr. Soc., 216, p. 923.CrossRefGoogle Scholar
Fabian, A.C., Crawford, C.S., Johnson, R.M. and Thomas, P.A., Mon. Not. R. astr. Soc., in press.Google Scholar
Foster, A.J., Ross, R.R. and Fabian, A.C.: 1987, Mon. Not. R. astr. Soc. 208, p. 29.Google Scholar
Fujimoto, M.Y., Sztajno, M., Lewin, W.H.G. and van Paradijs, J.: Astrophys. J. 319, p. 902.CrossRefGoogle Scholar
Hamilton, T.T. and Helfand, D.: 1987, Astrophys. J. 318, p. 93.CrossRefGoogle Scholar
Heise, J.: 1987, Proceedings of the Nato ASl “Hot Thin Plasmas in Astrophysics, in press.Google Scholar
Jones, C. and Forman, W., Jones, C. and Tucker, W.: 1985, Astrophys. J., 293, p. 102.Google Scholar
King, A.R., Watson, M.G. and Heise, J.: 1985, Nature, 313, p. 290.CrossRefGoogle Scholar
Lewin, W.H.G.: 1984, in “X-ray Astronomy 84”. Eds. M. Oda, and Giacconi, R., p. 157. ISAS.Google Scholar
Lewin, W.H.G.: 1986, in “The Physics of Accretion onto Compact Objects”. Eds. Mason, K., Watson, M.G. and White, N.E., p. 377, Springer-Verlag.Google Scholar
Lewin, W.H.G. et al: 1987 Astrophysics J., 319, p. 893.CrossRefGoogle Scholar
McClintock, J.E. and Remillard, R.A.: 1986, Astrophys. J., 308, p. 110.CrossRefGoogle Scholar
Mewe, R., Schrijver, C.J., Lemen, J.R. and Bentley, R.D.: 1986, Adv. Res., 6, p. 133.CrossRefGoogle Scholar
Nulsen, P.E., Stewart, G.C. and Fabian, A.C.: 1984, Mon. Not. R. astr., 208, p. 185.CrossRefGoogle Scholar
Paerels, F.B.S., Bleeker, J.A.M., Brinkman, A.C., Gronenschild, E.H.B.M., and Heise, J.: 1986, Ap. J., 308, p. 190.CrossRefGoogle Scholar
Pounds, K.A., Stanger, V.J., Turner, T.J. and King, A.R. and Czerny, B.: 1986a, Mon. Not. R. astr. Soc., 224, p. 443.CrossRefGoogle Scholar
Pounds, K.A., Turner, T.J. and Warwick, R.S.: 1986b, Mon. Not. R. astr. Soc., 221, 7P.CrossRefGoogle Scholar
Schrijver, C.J. and Mewe, R., 1985, in “Cool Stars, Stellar Systems and the Sun”, ed. Zeilik, and Gibson, , Springer-Verlag, p. 300.Google Scholar
Smith, A.: 1987, Proc IAU Colloquium 101.CrossRefGoogle Scholar
Stella, L., Priedhorsky, W. and White, N.E.: 1987, Astrophys. J., 312, L17.CrossRefGoogle Scholar
Sztajno, M. et al: 1985, Astrophys. J. 299, p. 487.CrossRefGoogle Scholar
Tananbaum, H. et al: 1986, Astrophys. J. 305, p. 57.CrossRefGoogle Scholar
Tennant, A.C., Fabian, A.C. and Shafer, R.A.: 1986, Mon. Not. R. astr. Soc., 221, 27P.CrossRefGoogle Scholar
Trinchieri, G. and Fabbiano, G.: 1985, Astrophys. J., 296, p. 447.CrossRefGoogle Scholar
Trumper, J.: 1984, in “X-ray and UV emission from AGN”, Eds. Brinkmann, W. and Trumper, J., p. 254. M.P.E., Garching.Google Scholar
Tsunemi, H., Yamashita, K., Masai, K., Hayakawa, S. and Koyama, K.: 1986, Astrophys. J., 306, p. 248.CrossRefGoogle Scholar
Turner, M.J.L. and Breedon, L.M.: 1984, Mon. Not. R. astr. Soc., 208, p. 29.CrossRefGoogle Scholar
Van der Klis, M. et al: 1985, Nature, 316, p. 225.CrossRefGoogle Scholar
Woerd, Van der et al: 1987, Astron. and Astrophys., 182, p. 219.Google Scholar
Van Paradijs, J. et al: 1986, Mon. Not. R. astr. Soc., 221, p. 617.CrossRefGoogle Scholar
Waki, I. et al: 1984, Pub. astr. Soc. Japan, 36, p. 819.Google Scholar
Watson, M.G. and King, A.R.: 1985, Mon. Not. R. astr., 212, p. 917.CrossRefGoogle Scholar
Watson, M.G., Stewart, G.C., Brinkmann, W. and King, A.R.: 1986, Mon. Not. R. astr. Soc., 222, p. 261.CrossRefGoogle Scholar
White, N.E. et al: 1984, Astrophys. J., 283, L9.CrossRefGoogle Scholar
White, N.E.: 1986, in “The Physics of Accretion onto Compact Objects”, Eds. Mason, K., Watson, M.G. and White, N.E. p. 377.Google Scholar
White, N.E., Culhane, J.L., Parmar, A.N., Kellet, B.J., Kahn, S. van der Oord, G.H.J., and Kuipers, J.: 1986, Ap. J., 301, p. 262.CrossRefGoogle Scholar
White, N.E., Shafer, R. and Parmar, A.N., 1987a, Proceedings of the 5th Cambridge Workshop, “Cool Stars, Stellar Systems and the Sun”, in press.Google Scholar
White, N.E., Culhane, J.L., Parmar, A.N. and Sweeney, M.A., 1987b, MNRAS.Google Scholar
Winckler, P.F., Canizares, C.R. and Bromley, B.C.: 1983, in Proc. IAU Symposium 101, “Supernova Remnants and their X-ray Emission”, p. 245. Reidel.Google Scholar
Worrall, D.M.: 1987, Astrophys. J., 318, p. 188.CrossRefGoogle Scholar