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Variable and Non-spherical Stellar Winds in Luminous Hot Stars pp 111–114Cite as

Inverse spectropolarimetric modelling of hot star wind structure and variability

  • Observations Of Non-spherical Winds
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Part of the book series: Lecture Notes in Physics ((LNP,volume 523))

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Author information

Authors and Affiliations

  1. Dept of Physics and Astronomy, University of Glasgow, G12 8QQ, UK

    John C. Brown & Richard Ignace

  2. INFN, Universita di Genova, Genova, Italy

    M. Piana

Authors
  1. John C. Brown
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  2. Richard Ignace
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  3. M. Piana
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Editor information

Bernhard Wolf Otmar Stahl Alex W. Fullerton

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© 1999 Springer-Verlag

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Brown, J.C., Ignace, R., Piana, M. (1999). Inverse spectropolarimetric modelling of hot star wind structure and variability. In: Wolf, B., Stahl, O., Fullerton, A.W. (eds) Variable and Non-spherical Stellar Winds in Luminous Hot Stars. Lecture Notes in Physics, vol 523. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0106363

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  • DOI: https://doi.org/10.1007/BFb0106363

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-65702-6

  • Online ISBN: 978-3-540-49062-3

  • eBook Packages: Springer Book Archive

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