Bridging model and observed stellar spectra

被引:2
作者
Prieto, C. Allende [1 ,2 ]
机构
[1] Inst Astrofis Canarias, Tenerife 38205, Spain
[2] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
关键词
techniques: spectroscopic; atlases; catalogues; stars: atmospheres; stars: fundamental parameters; galaxies: stellar content; NEWTON-TELESCOPE LIBRARY; DIGITAL SKY SURVEY; POPULATION SYNTHESIS; ATMOSPHERIC PARAMETERS; EMPIRICAL SPECTRA; ABSOLUTE FLUX; IRON-PROJECT; ATOMIC DATA; RESOLUTION; STARS;
D O I
10.1111/j.1365-2966.2010.17717.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Accurate model stellar fluxes are key for the analysis of observations of individual stars or stellar populations. Model spectra differ from real stellar spectra due to limitations of the input physical data and adopted simplifications, but can be empirically calibrated to maximize their resemblance to actual stellar spectra. We describe a least-squares procedure of general use and test it on the MILES library.
引用
收藏
页码:807 / 812
页数:6
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