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Optical Counterparts of HEAO-1 X-ray Sources

Published online by Cambridge University Press:  25 April 2016

D. A. H. Buckley ,
I. R. Tuohy  and
R. A. Remillard
D. A. H. Buckley
Affiliation:
Mount Stromio and Siding Spring Observatories, Australian National University
I. R. Tuohy
Affiliation:
Mount Stromio and Siding Spring Observatories, Australian National University
R. A. Remillard
Affiliation:
Massachusetts Institute of Technology
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Abstract

We present preliminary results of a search for the optical counterparts of faint but energetic (1-13 keV) X-ray sources observed by the HEAO-1 satellite. The objects we have identified include Active Galactic Nuclei, Cataclysmic Variables, Be Binaries, and RS CVn Systems. A description is also given of the identification techniques and the X-ray database, which represents the most recent flux-limited all-sky survey of hard X-ray sources.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 2 , 1985 , pp. 147 - 151
Copyright
Copyright © Astronomical Society of Australia 1985

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References

Bessell, M. S., 1985, To be submitted to Pub. Astron. Soc. Pacific. Buckley, D. A. H., Tuohy, I. R., Remillard, R., Bradt, H., and Schwartz, D., 1985a, In preparation.Google Scholar
Buckley, D. A. H., Tuohy, I. R., Remillard, R., Bradt, H., and Schwartz, D., 1985b, In preparation.Google Scholar
Bradt, H., and McClintock, J., 1983, Annu. Rev. Astron. Astrophys. 21, 13.Google Scholar
Clark, G. W., Li, F., and Van Paradijs, J., 1979, Astrophys. J., 227, 54.Google Scholar
Cordova, F. A., and Mason, K. O., in “Accretion Driven Stellar X-ray Sources”, eds. Lewin, W. H. G. and van den Heuvel, E. P. J. (Cambridge, England: Cambridge University Press) (1983).Google Scholar
Crampton, D., Hutchings, J., and Cowley, A., Astrophys. J. Lett., 1978, 223, L79 (1978).Google Scholar
Gursky, H., Bradt, H., Doxsey, R., Schwartz, D., Scharz, J., Dower, R., Fabiano, G., Griffiths, R. E., Johnson, M., Leach, R., Ramsey, A., and Spada, G., 1978, Astrophys. J., 223, 973.Google Scholar
Hall, D. S., in “Multiple Periodic Variable Stars”, 1976, IAU Colloq. No. 29, Part 1, 287.Google Scholar
Hutchings, J. B., Crampton, D., Cowley, A., and Osmer, P., 1977, Astrophys. J., 217, 186.Google Scholar
Hutchings, J. B., In “Galactic X-ray Sources”, eds. Sandford, P. W. Laskarides, P. and Salton, J. p.3 (Wiley) (1982).Google Scholar
Johnson, H. M., Astrophys. J., 243, 234.Google Scholar
Lamb, D. Q., in “Cataclysmic Variables and Low Mass X-ray Binaries”, eds. Lamb, D. Q. and Patterson, J. (ReidehDordrecht) (1985).Google Scholar
Margon, B., in “X-ray Astronomy”, eds. Baity, W. A. and Peterson, L. E. p.67 (Oxford:Pergamon Press) (1978).Google Scholar
Rappaport, S., and van den Heuvel, E. P. J., 1982, IAU Symp. 98, p. 327.Google Scholar
Remillard, R. A., Bradt, H. V., Buckley, D. A. H., Roberts, W., Schwartz, D. A., and Tuohy, I. R., 1986, Astrophys. J., in press.Google Scholar
Schmidt, M., and Green, R. F., 1983, Astrophys. J., 269, 352, (1983).CrossRefGoogle Scholar
Steiner, J. E., 1981, Astrophys. J., 250, 469.Google Scholar
Tuohy, I. R., Buckley, D. A. H., Remillard, R. A., Bradt, H. V., and Schwartz, D. A., 1985a, submitted to Astrophys. J., (1985a).Google Scholar
Tuohy, I. R., Buckley, D. A. H., Remillard, R. A., Bradt, H. V., and Schwartz, D. In Recent Results on Cataclysmic Variables, Proc. of the Bamberg ESA Workshop, ESA SP- 73 (1985b).Google Scholar
Walter, F. M., Charles, P. A., and Bowyer, C. S., 1978, Ap. J. Lett., 225, L119.Google Scholar
Warner, B., IAU Symp. No. 73 p. 85 (1976).Google Scholar
Warner, B., in “Cataclysmic Variables and Related Objects”, eds. Livio, M. and Shaviv, G., (Reidel:Dordrecht), p. 155, (1983).Google Scholar
Wood, K. S., Meekins, J. F., Yentic, D. J., Smathers, H. W., McNutt, D. P., Bleach, R. D., Byram, E. T., Chubb, T. A., Friedman, H., and Meidav, M., 1984, Astrophys. J. Suppl., 56, 507.Google Scholar