Infrared laboratory spectroscopy with astrophysical applications

被引：5
|
作者：
Nilsson, Hampus [1 ]
机构：
[1] Lund Univ, Lund Observ, SE-22100 Lund, Sweden
来源：
PHYSICA SCRIPTA | 2009年 / T134卷
关键词：
IRON-GROUP ELEMENTS; OSCILLATOR-STRENGTHS; CH-CYGNI; Y-II; ABUNDANCE; YTTRIUM; SPECTRA;
D O I：
10.1088/0031-8949/2009/T134/014009
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The infrared (IR) atomic spectral lines that can be observed in laboratory and astrophysical spectra depend both on the atomic structure and the physical conditions in which the atoms reside. This is a brief review of IR laboratory spectroscopy, discussing which lines in the wavelength interval 1-5 mu m can be expected to be seen in different astrophysical sources.
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页数：7
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