Grid/NLTE
收藏官方服务：
资源简介：
Non-LTE departure coefficients for late-type stars. For this version, see Ag I model atom and the 3D non-LTE solar silver abundance (Caliskan, Amarsi, Jönsson, Grevesse, and Sahoo, A&A, in press), and references therein. The methods were first presented in Non-LTE departure coefficients for large spectroscopic surveys (Amarsi et al., A&A, 2020, 642, A62).
提供机构：
Zenodo创建时间：
2020-06-11
