Constrained fitting of disentangled binary star spectra: application to V615 Persei in the open cluster h Persei
Year: 2010
Type: article
Abstract: Context. Using the technique of spectral disentangling, it is possible to determine the individual spectra of the components of a multiple star system from composite spectra observed at a range of orbital phases. This method has several advantages: it is unaffected by line blending, does not use template spectra, and returns individual component spectra with very high signal-to-noise ratios.
Source: Astronomy and Astrophysics
Authors: E. Tamajo, K. Pavlovski, J. Southworth
Institutions: University of Zagreb, Keele University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2059008569
