The Contact Binary AE Phoenicis — an Analysis from Deconvoluted Spectra
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.
KeywordsRotational Velocity Spectroscopic Observation Roche Lobe Double Star DECONVOLUTED Spectrum
Unable to display preview. Download preview PDF.