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Astron. Astrophys. Suppl. Ser.
Volume 122, Number 3, May_I 1997
Page(s) 581 - 584
DOI: 10.1051/aas:1997102

A&A Supplement series, Vol. 122, May I 1997, 581-584

Received May 20; Accepted August 21, 1996

Relative line photometry of eclipsing binaries

P. Hadrava

Astronomical Institute, Academy of Sciences of the Czech Republic, 251 65 Ondrejov, Czech Republic,


A new method of "line-photometry'' using the changes of line intensities for determination of light curves in eclipsing binaries is described. This method is based on a generalization of the method of spectrum decomposition by Fourier transform performed by the code KOREL for spectrum disentangling.

keywords: line profiles -- stars: binaries spectroscopic -- methods: numerical

Copyright by the European Southern Observatory (ESO)

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