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The Contact Binary AE Phoenicis - An Analysis from Deconvoluted Spectra
1984
International Astronomical Union Colloquium
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AbstractA 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.
doi:10.1017/s0252921100088515
fatcat:ejyppwdcmncg3l57cqum6ollvy