Sco X-1 |
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Authors: | Senori Miyamoto Masaru Matsuoka |
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Institution: | (1) Institute of Space and Aeronautical Science, University of Tokyo, Komaba, Meguro-ku, 153 Tokyo, Japan;(2) Present address: Dept. of Physics, Faculty of Science, Osaka University, Machikaneyama-cho, 560 Toyonaka-shi, Osaka, Japan |
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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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