Relative line photometry of eclipsing binaries.
Abstract
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.
- Publication:
-
Astronomy and Astrophysics Supplement Series
- Pub Date:
- May 1997
- DOI:
- 10.1051/aas:1997102
- Bibcode:
- 1997A&AS..122..581H
- Keywords:
-
- LINE PROFILES;
- STARS: BINARIES SPECTROSCOPIC;
- METHODS: NUMERICAL