Abundances from disentangled component spectra: the eclipsing binary V578 Mon

Chemical abundances of the early–B type components of the binary V578 Mon are derived from disentangled component spectra. This is a pilot study showing that, even with moderately high line-broadening, metal abundances can be derived from disentangled spectra with a precision of 0.1 dex, differentia...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2005-08, Vol.439 (1), p.309-315
Hauptverfasser:	Pavlovski, K., Hensberge, H.
Format:	Artikel
Sprache:	eng
Schlagworte:	open clusters and associations: individual: NGC 2244 stars: abundances stars: binaries: spectroscopic stars: individual: V578 Mon (HDE 259 135) techniques: spectroscopic
Online-Zugang:	Volltext
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