中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
evolutionofm81withexponentiallydecreasingstarformationrateofpegase

文献类型:期刊论文

作者Li Jiuli; Zhou Xu; Ma Jun; Chen Jiansheng
刊名chinesejournalofastronomyandastrophysics
出版日期2004
卷号4期号:2页码:143
ISSN号1009-9271
英文摘要Based on the large field multicolor observations of Beijing-Arizona-Taiwan-Connecticut (BATC) program, we obtain the spectral energy distribution (SED) for individual regions of M81. We study the structure and evolution of M81 with an evolutionary population synthesis (EPS) model, PEGASE. We find that the exponentially deceasing star formation rate (SFR) with star formation scale 3 Gyr (hereafter Exp, T = 3 Gyr) gives the best agreement between the model predictions and the observed SEDs. We then obtain the structure, age distribution and evolutionary history of M81. There is a clear age gradient between the central and outer regions. The populations in the central regions are older than 7 Gyr, those in the outer regions are younger, at about 4.5 Gyr. The youngest components in the spiral arms have ages of about 2.5 Gyr or less.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/47096]  
专题中国科学院国家天文台
作者单位中国科学院国家天文台
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GB/T 7714
Li Jiuli,Zhou Xu,Ma Jun,et al. evolutionofm81withexponentiallydecreasingstarformationrateofpegase[J]. chinesejournalofastronomyandastrophysics,2004,4(2):143.
APA Li Jiuli,Zhou Xu,Ma Jun,&Chen Jiansheng.(2004).evolutionofm81withexponentiallydecreasingstarformationrateofpegase.chinesejournalofastronomyandastrophysics,4(2),143.
MLA Li Jiuli,et al."evolutionofm81withexponentiallydecreasingstarformationrateofpegase".chinesejournalofastronomyandastrophysics 4.2(2004):143.

入库方式: OAI收割

来源:国家天文台

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