The contact binary AE Phoenicis - an analysis from deconvoluted spectra

Details The contact binary AE Phoenicis - an analysis from deconvoluted spectra The contact binary AE Phoenicis - an analysis from deconvoluted spectra

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..157b&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

2

Convolution Integrals, Eclipsing Binary Stars, Spectrum Analysis, Stellar Spectra, Stellar Spectrophotometry, Angular Velocity, Orbital Elements, Stellar Models

Scientific paper

A method is described for an analysis of deconvoluted stellar spectra, and applied to new spectroscopic observations of the close eclipsing system AE Phoenicis, 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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