中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Evolutionary Population Synthesis for Single Stellar Populations

文献类型:期刊论文

作者Jarrod R Hurley2; Zhang Fenghui1; Han Zhanwen1; Li Lifang1
刊名Chinese Physics Letters
出版日期2002
卷号19期号:11页码:1734
ISSN号0256-307X
英文摘要Using the evolutionary population synthesis technique, we present the latest integrated colours for instantaneous burst single stellar populations (SSPs) of different metallicities and we investigate their colour evolution. Unlike previous research, we adopt the stellar evolutionary models that employ, amongst other things, recent opacities and a revised equation of state (EOS), and include evolutionary processes such as convective overshooting, thermal pulses and dredge-up. The models are used in the convenient form of analytical fitting functions. In addition, we use the BaSeL model for the library of stellar spectra. This model provides an extensive low-resolution theoretical flux distribution and UBVRIJHKLM colours, which have been calibrated empirically or semi-empirically, for a wide range of stellar parameters.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/46757]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024
推荐引用方式
GB/T 7714
Jarrod R Hurley,Zhang Fenghui,Han Zhanwen,et al. Evolutionary Population Synthesis for Single Stellar Populations[J]. Chinese Physics Letters,2002,19(11):1734.
APA Jarrod R Hurley,Zhang Fenghui,Han Zhanwen,&Li Lifang.(2002).Evolutionary Population Synthesis for Single Stellar Populations.Chinese Physics Letters,19(11),1734.
MLA Jarrod R Hurley,et al."Evolutionary Population Synthesis for Single Stellar Populations".Chinese Physics Letters 19.11(2002):1734.

入库方式: OAI收割

来源:国家天文台

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