AN INTRODUCTION TO THE SUBJECT OF THIS WORKSHOP

被引：1
|
作者：
Mashonkina, L. [1 ]
机构：
[1] Russian Acad Sci, Inst Astron, Moscow 119017, Russia
来源：
NON-LTE LINE FORMATION FOR TRACE ELEMENTS IN STELLAR ATMOSPHERES | 2010年 / 43卷
关键词：
LINE-BLANKETED MODEL; STELLAR ATMOSPHERE PROGRAM; NON-LTE; PARALLEL IMPLEMENTATION; STARS; OPACITY;
D O I：
10.1051/eas/1043003
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A brief review of the terms and definitions related to stellar atmosphere modelling and spectral line formation is presented. In particular, two topics are discussed: the chemical elements that can be treated in a given atmosphere as trace elements, and the scattering processes that are taken into account in line formation modelling.
引用
收藏
页码：33 / 42
页数：10
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