Disentangling of spectra of multiple stars

Details Disentangling of spectra of multiple stars Disentangling of spectra of multiple stars

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318...86h&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

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19

Scientific paper

The method of disentangling, which consists of simultaneous decomposition of spectra of multiple stellar systems and solution of orbital parameters has proved to be an effective way of determination of physical parameters of the component stars, applicable even for cases with highly blended spectral lines. The basic principle of disentangling and its relation to several other spectroscopic methods is reviewed here and a new generalization of the method for intrinsic line-profile variability is introduced.

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