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The complementarity of Doppler imaging and photometric starspot modelling

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Abstract

Certain essential formal similarities between the modelling of photometric maculation effects and spectrometric Doppler imaging are pointed out. This parallelism opens the way to a methodological approach to Doppler imaging on quite parallel lines to the authors' studies of stars that exhibit photometric maculation waves. The information content of either form of data set is thence compared.

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Authors and Affiliations

  1. Carter Observatory, Wellington, New Zealand

    E. Budding

  2. Institute for Astrophysics, Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA

    M. Zeilik

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  1. E. Budding
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  2. M. Zeilik
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Budding, E., Zeilik, M. The complementarity of Doppler imaging and photometric starspot modelling. Astrophys Space Sci 222, 181–190 (1994). https://doi.org/10.1007/BF00627092

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  • DOI: https://doi.org/10.1007/BF00627092

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