Detailed Opacity Calculations for Astrophysical Applications

Detailed Opacity Calculations for Astrophysical Applications

Nowadays, several opacity codes are able to provide data for stellar structure models, but the computed opacities may show significant differences. In this work, we present state-of-the-art precise spectral opacity calculations, illustrated by stellar applications. The essential role of laboratory e...

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Autors principals:	Jean-Christophe Pain, Franck Gilleron, Maxime Comet
Format:	Article
Idioma:	English
Publicat:	MDPI AG 2017-05-01
Col·lecció:	Atoms
Matèries:	atomic physics spectroscopy astrophysics β Cephei white dwarfs stellar envelopes radiative zone of the Sun
Accés en línia:	http://www.mdpi.com/2218-2004/5/2/22

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