Abstract
A SYSTEMATIC search is being made for the optical counterparts of the better localized X-ray sources. Here we report a preliminary result of the study of GX 17 + 2 (2U 1813–14).
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Tananbaum, H., Gursky, H., Kellog, E., and Giacconi, R., Astrophys. J. Lett. 168, L25 (1971).
Kunkel, W., Osmer, P., Smith, M., Hoag, A., Schroeder, D., Hiltner, W. A., Bradt, H., Rapport, S., and Schnopper, H. W., Astrophys. J. Lett., 161, L169 (1970).
Schnopper, H. W., Bradt, H. V., Rapport, S., Boughan, E., Burnett, B., Doxsey, R., Mayer, W., and Watt, S., Astrophys. J. Lett., 161, H61 (1970).
Hjellming, R. M., and Wade, C. M., Astrophys. J. Lett., 168, L21 (1971).
Brown, R. L., and Gould, R. J., Phys. Rev., D, 1, 2252 (1970).
Reina, C., thesis, Univ. Milano (1972).
Feiten, J. E., and Rees, M. J., Astron. Astrophys., 17, 226 (1972).
Gorenstein, P., Giacconi, R., and Gursky, H., Astrophys. J. Lett., 150, L85 (1967).
Ilovaisky, S. A., Astron. Astrophys., 11, 134 (1971).
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TARENGHI, M., REINA, C. Optical Identification of GX 17 + 2. Nature Physical Science 240, 53–54 (1972). https://doi.org/10.1038/physci240053a0
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DOI: https://doi.org/10.1038/physci240053a0
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