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Short time-scale changes in the V-band light-curve of II Peg: Flare, companion or prominence?

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Surface Inhomogeneities on Late-Type Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 397))

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Authors and Affiliations

  1. Armagh Observatory, BT61 9DG, Armagh, N. Ireland

    J. G. Doyle & H. M. Murphy

  2. Astrophysics Div., Rutherford Appleton Lab., Chilton, Didcot, Oxon., England

    G. E. Bromage

  3. Astronomy Center, University of Sussex, BN1 0QH, Falmer, Brighton, England

    A. C. Cameron

  4. South African Astronomical Obser., PO Box 9, 7935, Observatory, South Africa

    D. W. Kilkenny & F. van Wyk

  5. Dept. of Astronomy, Pedagogical University, PL 30-084, Krakow, Poland

    J. Krzesinski & G. Pajdosz

  6. NASA/Goddard Space Flight Center, Bld. 21, 20771, Greenbelt, MD, USA

    J. E. Neff

Authors
  1. J. G. Doyle
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  2. G. E. Bromage
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  3. A. C. Cameron
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  4. D. W. Kilkenny
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  5. J. Krzesinski
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  6. H. M. Murphy
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  7. J. E. Neff
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  8. G. Pajdosz
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  9. F. van Wyk
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Patrick B. Byrne Dermott J. Mullan

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© 1992 Springer-Verlag

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Doyle, J.G. et al. (1992). Short time-scale changes in the V-band light-curve of II Peg: Flare, companion or prominence?. In: Byrne, P.B., Mullan, D.J. (eds) Surface Inhomogeneities on Late-Type Stars. Lecture Notes in Physics, vol 397. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55310-X_168

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  • DOI: https://doi.org/10.1007/3-540-55310-X_168

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-55310-6

  • Online ISBN: 978-3-540-47025-0

  • eBook Packages: Springer Book Archive

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