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A spectroscopic study of Epsilon Aurigae

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Abstract

Epsilon Aurigae has been observed during ingress and totality between 1982 and 1983 at Okayama. Analyses of profiles of Hα line and of radial velocities of neutral hydrogen and metals show that the secondary component consists of at least three parts in structure.

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Authors and Affiliations

  1. Department of Astronomy, Kyoto University, Kyoto, Japan

    Mamoru Saitō

  2. Kyoto Gakuen University, Kameoka, Kyoto, Japan

    Shusaku Kawabata

  3. National Science Museum, Ueno Park, Tokyo, Japan

    Keiich Saijo

  4. Tokyo Astronomical Observatory, Mitaka, Tokyo, Japan

    Hideo Sato

Authors
  1. Mamoru Saitō
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  2. Shusaku Kawabata
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  3. Keiich Saijo
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  4. Hideo Sato
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Saitō, M., Kawabata, S., Saijo, K. et al. A spectroscopic study of Epsilon Aurigae. Astrophys Space Sci 99, 269–272 (1984). https://doi.org/10.1007/BF00650249

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  • DOI: https://doi.org/10.1007/BF00650249

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