Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-24T16:05:43.402Z Has data issue: false hasContentIssue false
  • English
  • Français

RS CVn Systems: The High Energy Picture

Published online by Cambridge University Press:  12 April 2016

P.A. Charles
P.A. Charles*
Affiliation:
Department of Astrophysics, University of Oxford

Abstract

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.

The discovery of X-ray emission from RS CVn systems by HEAO-1 and subsequent surveys by the Einstein Observatory have shown that these close binaries exhibit greatly enhanced coronal activity. Here we review the 3 main observational areas: (1) results of the X-ray surveys of RS CVn systems and other late-type stars which indicate how the X-ray luminosity is correlated with the binary period (and hence stellar rotation) and other coronal activity indicators. This will be discussed in the context of scaled models of the solar corona; (2) X-ray spectroscopy of the most active systems which show multitemperature spectra and line emission consistent with solar abundances of the heavy elements; (3) observations of X-ray “flare-type” activity that has been associated with several RS CVn systems.

Type
Session III: Observed Activity in Related Objects
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 415 - 427
Copyright
Copyright © Reidel 1983

References

REFERENCES

Agrawal, P., Riegler, G.R. & White, N.E.: 1981, M.N.R.A.S., 196, 73P.Google Scholar
Booth, L. & Charles, P.A.: 1982, M.N.R.A.S., (in press).Google Scholar
Cash, W., Bowyer, S., Charles, P., Lampton, M., Garmire, G. & Riegler, G. : 1978, Ap.J., 223, L21.Google Scholar
Charles, P., Walter, F. & Bowyer, S.: 1979, Nature, 282, 691.CrossRefGoogle Scholar
Dorren, J.D., Siah, M.J., Guinan, E.F. & McCook, G.P.: 1981, A.J., 86,572.CrossRefGoogle Scholar
Eaton, J.A. & Hall, D.S.: 1979, Ap.J., 227, 907.CrossRefGoogle Scholar
Feldman, P.A., Taylor, A.R., Gregory, P.C., Seaquist, E.R., Balouek, T.J. & Cohen, N.L.: 1978, A.J. 83, 1471.CrossRefGoogle Scholar
Garcia, M., Baliunas, S.L., Conroy, M.,Johnston, M.D., Ralph, E.,Roberts, W., Schwartz, D.A. & Tonry, J.: 1980, Ap.J. 240, L107Google Scholar
Gibson, D.M., Hjellming, R.M. & Owen, F.N.: 1975, Ap.J., 200, L99.Google Scholar
Gronenschild, E.H.B.M., Mewe, R., Westergaard, N.J., Heise, J., Seward, F.D., Chlebowski, T., Kuin, N.P.M., Brinkman, A.C., Dijkstra, J.H. & Schnopper, H.W.: Sp.Sci.Rev. 30, 185.CrossRefGoogle Scholar
Hall, D.S.: 1972, P.A.S.P., 84, 323.CrossRefGoogle Scholar
Hall, D.S.: 1976, IAU Colloquium# 29, 287, in Multiple Periodic Variable Stars, ed. by Fitch, W.S. (Holland-Reidel).Google Scholar
Hall, D.S., Henry, G.W. & Louth, H. : 1982, Ap.J., 257, L91.Google Scholar
Hoffleit, D. & Jaschek, C.: 1982, Bright Star Catalogue, 4th Edition, Yale University Observatory.Google Scholar
Joyce, R.M., Becker, R.H., Birsa, F.B., Holt, S.S. & Noordzy, M.P.: 1978, IEEE Trans.Nucl.Sci. 25, 453.CrossRefGoogle Scholar
Kimble, R.A., Kahn, S.M. & Bowyer, S.: 1981, Ap.J., 251, 585.CrossRefGoogle Scholar
McHardy, I.M., Pye, J.P., Fairall, A.P., Caldwell, J. & Spencer-, Jones J.: 1982, M.N.R.A.S. (submitted)Google Scholar
Mewe, R., Schrijver, C.J. & Zwaan, C.: 1981, Sp.Sci.Rev. 30, 191.CrossRefGoogle Scholar
Pallavicini, R., Golub, L., Rosner, R., Vaiana, G.S., Ayres, T. & Linsky, J.L.: 1981, Ap.J., 248, 279 (PAL).CrossRefGoogle Scholar
Popper, D.: 1980, in Close Binary Stars: Observations and Interpretation ed. Plavec, et al (Boston: Reidei) p.387.Google Scholar
Rosner, R., Tucker, W.H. & Vaiana, G.S.: 1978, Ap.J., 220, 643 (RTV).CrossRefGoogle Scholar
Rothschild, R., Boldt, E., Holt, S., Serlemitsos, P., Gannire, G., Agrawal, P., Riegler, G., Bowyer, S. & Lampton, M.: 1979, Sp.Sci.Instr. 4, 269.Google Scholar
Rucinski, S.M.: 1977, PASP 89, 280.CrossRefGoogle Scholar
Schrijver, C.J., Mewe, R. & Zwaan, C.: 1982, Astron.Astrophys.(submitted) (SMZ).Google Scholar
Schwartz, D.A., Bradt, H., Briel, U., Doxsey, R.E., Fabbiano, G., Griffiths, R.E., Johnston, M.D. &Margon, B., 1979, A.J. 84, 1560.CrossRefGoogle Scholar
Schwartz, D.A., Garcia, M., Ralph, E., Doxsey, R.E., Johnston, M.D., Lawrence, A., McHardy, I.M. & Pye, J.P.: 1981, M.N.R.A.S. 196, 95.CrossRefGoogle Scholar
Skumanich, A.: 1972, Ap.J., 171, 565.CrossRefGoogle Scholar
Simon, T. & Linsky, J.L.: 1980, Ap.J., 241, 759.CrossRefGoogle Scholar
Swank, J.H. & White, N.E.: 1980, in Cool Stars, Stellar Systems and the Sun ed.Dupree, A.K. , SAO Sp.Rep. 389, 47.Google Scholar
Swank, J.H., White, N.E., Holt, S.S. & Becker, R.H.: 1981, Ap.J., 246,208.CrossRefGoogle Scholar
Walter, F.M.: 1981, Ap.J., 245, 677.CrossRefGoogle Scholar
Walter, F.M.: 1982, Ap.J., 253, 745.CrossRefGoogle Scholar
Walter, F.M. & Bowyer, S., 1981, Ap.J., 245, 671 (WB).CrossRefGoogle Scholar
Walter, F.M., Cash, W., Charles, P.A. & Bowyer, S.: 1980, Ap.J. 236, 212.CrossRefGoogle Scholar
Walter, F., Charles, P. & Bowyer, S.: 1978, Ap.J.Letters 225, L119.CrossRefGoogle Scholar
White, N.E., Holt, S.S., Becker, R.H., Boldt, E.A. & Serlemitsos, P.J.: 1980, Ap.J., 239, L69.CrossRefGoogle Scholar
White, N.E., Sanford, P.W. & Weiler, E.J.: 1978, Nature, 274, 569.CrossRefGoogle Scholar