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UV Energy Distributions of Active Cool Stars

  • Conference paper
Fundamental Stellar Properties: The Interaction Between Observation and Theory

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 189))

Abstract

We present semi-empirical models based on the ”minimum-temperature-concept” in order to provide a description of the UV spectra of solar type stars consistent with the observational data.

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References

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Author information

Authors and Affiliations

  1. Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34131, Trieste, Italy

    C. Morossi & M. Franchini

  2. Dipartimento di Astronomia, Università degli Studi di Trieste, Via Tiepolo 11, I-34131, Trieste, Italy

    M. L. Malagnini

Authors
  1. C. Morossi
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  2. M. Franchini
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  3. M. L. Malagnini
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Editor information

Editors and Affiliations

  1. School of Physics, University of Sydney, Australia

    T. R. Bedding , A. J. Booth  & J. Davis ,  & 

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© 1997 Springer Science+Business Media Dordrecht

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Morossi, C., Franchini, M., Malagnini, M.L. (1997). UV Energy Distributions of Active Cool Stars. In: Bedding, T.R., Booth, A.J., Davis, J. (eds) Fundamental Stellar Properties: The Interaction Between Observation and Theory. International Astronomical Union / Union Astronomique Internationale, vol 189. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5602-8_14

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  • DOI: https://doi.org/10.1007/978-94-011-5602-8_14

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-4652-4

  • Online ISBN: 978-94-011-5602-8

  • eBook Packages: Springer Book Archive

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