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Stellar X-Ray Sources

Published online by Cambridge University Press:  14 August 2015

Harvey D. Tananbaum
Harvey D. Tananbaum*
Affiliation:
American Science & Engineering, Cambridge, Mass., U.S.A.

Abstract

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Data are presented for Cygnus X-1, Cygnus X-3, and Scorpius X-1 from radio to X-ray wavelengths. The evidence for Cygnus X-1's being a black hole is now quite convincing. New data for Cygnus X-3 show the presence of X-ray activity at the time of the giant radio outburst. The data for Scorpius X-1 show a close correlation between the X-ray and optical behavior, but coverage was not sufficiently complete to fully assess the relationship (if any) between the X-ray and optical emission and the radio emission.

Type
Part 4: Stellar and Circumstellar Sources
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 383 - 399
Copyright
Copyright © Reidel 1974 

References

Becklin, E. E., Hawkins, F. J., Mason, K. O., Matthews, K., Neugebauer, G., Sanford, P. W., and Wynn-Williams, C. G.: 1973, preprint.Google Scholar
Bolton, C. T.: 1972a, Nature 235, 271.CrossRefGoogle Scholar
Bolton, C. T.: 1972b, Nature Phys. Sci. 240, 124.Google Scholar
Braes, L. and Miley, G. K.: 1971, Nature 232, 246.CrossRefGoogle Scholar
Bregman, J., Butler, D., Kemper, E., Koski, A., Kraft, R. P., and Stone, R. P. S.: 1973, preprint.Google Scholar
Canizares, C. R., McClintock, J. E., Clark, G. W., Lewin, W. H. G., Schnopper, H. W., and Sprott, G. F.: 1973, Nature Phys. Sci. 241, 28.CrossRefGoogle Scholar
Cherepaschuk, A. M., Lyutiy, V. M., and Sunyaev, R. A.: 1973, Astron. Zh. 50, 3.Google Scholar
Faulkner, J.: 1973, Tucson Workshop on Compact X-Ray Sources.Google Scholar
Gregory, P. C., Kronberg, P. P., Seaquist, E. R., Hughes, V. A., Woodsworth, A., Viner, M. R., and Retallack, D.: 1972, Nature Phys. Sci. 239, 440.Google Scholar
Gursky, H.: 1973, private communication.Google Scholar
Hiltner, W. A. and Mook, D. W.: 1970, Ann. Rev. Astron. Astrophys. 8, 139.Google Scholar
Hjellming, R. M.: 1973, Astrophys. J. Letters 182, L29.Google Scholar
Hjellming, R. M. and Wade, C. M.: 1971, Astrophys. J. Letters 168, L21.Google Scholar
Holt, S., Boldt, E., Schwartz, D., Serlemitsos, P., and Bleach, R.: 1971, Astrophys. J. Letters 166, L65.Google Scholar
Kitamura, T., Matsuoka, M., Miyamoto, S., Nakagawa, M., Oda, M., Ogawara, Y., Takagishi, K., Rao, U. R., Chitnis, E. V., Jayanthi, U. B., Prakasa-Rao, A. S., and Bhandari, S. M.: 1971, Astrophys. Space Sci. 12, 378.CrossRefGoogle Scholar
Margon, B., Bowyer, S., and Stone, R.: 1973, Astrophys. J. Letters, to be published.Google Scholar
Mauder, H.: 1973, Astron. Astrophys., to be published.Google Scholar
Parsignault, D. R., Gursky, H., Kellogg, E. M., Matilsky, T., Murray, S., Schreier, E., Tananbaum, H., Giacconi, R., and Brinkman, A. C.: 1972, Nature 239, 123.Google Scholar
Rappaport, S., Doxsey, R., and Zaumen, W.: 1971a, Astrophys. J. Letters 168, L43.Google Scholar
Rappaport, S., Zaumen, W., and Doxsey, R.: 1971b, Astrophys. J. Letters 168, L17.Google Scholar
Shulman, S., Fritz, G., Meekins, J., and Friedman, H.: 1971, Astrophys. J. Letters 168, 449.Google Scholar
Trimble, V., Rose, W. K., and Weber, J.: 1973, Monthly Notices Roy. Astron. Soc. 162, 1.Google Scholar
Tucker, W.: 1973, private communication.Google Scholar
Webster, B. L. and Murdin, P.: 1972, Nature 235, 37.Google Scholar