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The contact binary AE phoenicis — An analysis from deconvoluted spectra

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Abstract

A method is described for an analysis of deconvoluted stellar spectra, and applied to new spectroscopic observations of the close eclipsing system AE Phuenicis, obtained with the 1.52 m telescope of the Southern European Observatory at La Silla, Chile, Results are presented for the rotational velocities of this variable, together with a proposed model of the system.

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  1. Universitäts-Sternwarte Bonn, F.R.G.

    H. J. Becker

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  1. H. J. Becker
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Becker, H.J. The contact binary AE phoenicis — An analysis from deconvoluted spectra. Astrophys Space Sci 99, 157–161 (1984). https://doi.org/10.1007/BF00650240

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  • DOI: https://doi.org/10.1007/BF00650240

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