A&A Supplement series, Vol. 122, May I 1997, 581-584
Received May 20; Accepted August 21, 1996
P. HadravaAstronomical Institute, Academy of Sciences of the Czech Republic, 251 65 Ondrejov, Czech Republic, firstname.lastname@example.org
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