The Contact Binary AE Phoenicis — an Analysis from Deconvoluted Spectra

  • H. J. Becker


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.


Rotational Velocity Spectroscopic Observation Roche Lobe Double Star DECONVOLUTED Spectrum 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1984

Authors and Affiliations

  • H. J. Becker
    • 1
  1. 1.Universitäts-Sternwarte BonnGermany

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