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Sco X-1

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Abstract

The physical properties of X-ray, optical and radio emissions from Sco X-1 are reviewed. Sco X-1 is a typical X-ray source which has an optically thick hot plasma. The observational spectra of X-ray and optical emissions are consistent with theoretical ones from the hot plasma, but the radio emission shows a non-thermal feature. The restrictive conditions for the model of Sco X-1 are discussed from the observational facts. In spite of numerous observational facts on Sco X-1 further detailed and elaborate studies are necessary to understand this object and general compact X-ray sources comprehensively.

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  1. Senori Miyamoto

    Present address: Dept. of Physics, Faculty of Science, Osaka University, Machikaneyama-cho, 560, Toyonaka-shi, Osaka, Japan

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  1. Institute of Space and Aeronautical Science, University of Tokyo, Komaba, Meguro-ku, 153, Tokyo, Japan

    Senori Miyamoto & Masaru Matsuoka

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Miyamoto, S., Matsuoka, M. Sco X-1. Space Sci Rev 20, 687–755 (1977). https://doi.org/10.1007/BF02431834

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