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Late-Type Stars and Close Binaries

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The Astrophysics of Emission-Line Stars

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 342))

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Abstract

Late-type stars are generally characterized by the chromospheric structure showing active phenomena observable by the formation of emission lines and emission of X-ray and UV radiations. In the optical region, most ubiquitous emission lines are CaII H, K lines, while Hα line appears in fully developed chromospheres. In this section we consider the basic chromospheric activities by focusing to the CaII H, K emission lines.

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Authors and Affiliations

  1. Kyoto University, Personal: 1–10, Toganoo Hashimoto, Yawata, Kyoto, 614-8322, Japan

    Tomokazu Kogure (Emeritus Professor of Astronomy)

  2. Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan, China

    Kam-Ching Leung (Professor of Physics and Astronomy)

  3. Department of Physics & Astronomy, University of Nebraska-Lincoln, Lincoln, NE, USA

    Kam-Ching Leung (Professor of Physics and Astronomy)

  4. Brace Laboratory, Lincoln 68588-0111, 1186, USA

    Kam-Ching Leung (Professor of Physics and Astronomy)

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Kogure, T., Leung, KC. (2007). Late-Type Stars and Close Binaries. In: The Astrophysics of Emission-Line Stars. Astrophysics and Space Science Library, vol 342. Springer, New York, NY. https://doi.org/10.1007/978-0-387-68995-1_6

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