Quantitative Spectroscopy of Close Binary Stars (CROSBI ID 586192)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Pavlovski, Krešimir ; Southworth, John
engleski
Quantitative Spectroscopy of Close Binary Stars
The method of spectral disentangling has now created the opportunity for studying the chemical composition in previously inaccessible components of binary and multiple stars. This in turn makes it possible to trace their chemical evolution, a vital aspect in understanding the evolution of stellar systems. We review different ways to reconstruct individual spectra from eclipsing and non-eclipsing systems, and then concentrate on some recent applications to detached binaries with high-mass and intermediate-mass stars, and Algol-type mass-transfer systems.
binary stars; spectroscopy; stellar atmospheres; chemical composition
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Podaci o prilogu
359-364.
2012.
objavljeno
Podaci o matičnoj publikaciji
From Interacting Binaries to Exoplanets: Essential Modeling Tools, Proceedings IAU Symposium 282
Richards, Mercedes T. ; Hubeny, Ivan
Cambridge: Cambridge University Press
Podaci o skupu
Nepoznat skup
pozvano predavanje
29.02.1904-29.02.2096