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Laboratory identification of the 3P1,2 - 5S O2 intersystem lines of S III

  • 2. Rotation and Activity in Main Sequence Stars
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Cool Stars, Stellar Systems, and the Sun

Part of the book series: Lecture Notes in Physics ((LNP,volume 193))

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Authors and Affiliations

  1. Harvard-Smithsonian Center for Astrophysics, USA

    Peter L. Smith

  2. Physics Department, Lund University, UK

    C. E. Magnusson & P. O. Zetterberg

Authors
  1. Peter L. Smith
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  2. C. E. Magnusson
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  3. P. O. Zetterberg
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Sallie L. Baliunas Lee Hartmann

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© 1984 Springer-Verlag

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Smith, P.L., Magnusson, C.E., Zetterberg, P.O. (1984). Laboratory identification of the 3P1,2 - 5S O2 intersystem lines of S III. In: Baliunas, S.L., Hartmann, L. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 193. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-12907-3_199

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  • DOI: https://doi.org/10.1007/3-540-12907-3_199

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-12907-3

  • Online ISBN: 978-3-540-38785-5

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