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...
المؤلفون الرئيسيون: | Jean-Christophe Pain, Franck Gilleron, Maxime Comet |
---|---|
التنسيق: | مقال |
اللغة: | English |
منشور في: |
MDPI AG
2017-05-01
|
سلاسل: | Atoms |
الموضوعات: | |
الوصول للمادة أونلاين: | http://www.mdpi.com/2218-2004/5/2/22 |
مواد مشابهة
-
Solar astrophysics /
حسب: Foukal, Peter V.
منشور في: (2013) -
Solar astrophysics /
حسب: 376027 Foukal, Peter
منشور في: (2004) -
Laser-Plasma and Self-Absorption Measurements with Applications to Analysis of Atomic and Molecular Stellar Astrophysics Spectra
حسب: Christian G. Parigger, وآخرون
منشور في: (2019-07-01) -
Carbon–Oxygen Phase Separation in Modules for Experiments in Stellar Astrophysics (MESA) White Dwarf Models
حسب: Evan B. Bauer
منشور في: (2023-01-01) -
Seismic Signatures of the 12C(α, γ)16O Reaction Rate in White Dwarf Models with Overshooting
حسب: Morgan T. Chidester, وآخرون
منشور في: (2023-01-01)