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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© 1984 D. Reidel Publishing Company, Dordrecht, Holland
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Becker, H.J. (1984). The Contact Binary AE Phoenicis — an Analysis from Deconvoluted Spectra. In: Hidayat, B., Kopal, Z., Rahe, J. (eds) Double Stars, Physical Properties and Generic Relations. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6372-6_16
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DOI: https://doi.org/10.1007/978-94-009-6372-6_16
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-6374-0
Online ISBN: 978-94-009-6372-6
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