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“Star as a sun” observations in seismology of distant stars

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Abstract

The paper gives a brief description of a new procedure for seismology of pulsating CP2-stars. In analogy with the solar observations, this sensitive procedure permits one to carry out the spatial filtration of low, intermediate and high degree nonradial modes and uses periodic spatial filters associated with surface inhomogenities in the distribution of chemical elements. The possibilities of this procedure and its observational peculiarities are discussed.

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Authors and Affiliations

  1. Astronomical Observatory of Odessa State University, Shevchenko Park, 270014, Odessa, Ukraine

    D. E. Mkrtichian

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  1. D. E. Mkrtichian
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Mkrtichian, D.E. “Star as a sun” observations in seismology of distant stars. Sol Phys 152, 275–282 (1994). https://doi.org/10.1007/BF01473215

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  • DOI: https://doi.org/10.1007/BF01473215

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