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星系金属丰度的研究进展(Ⅱ):光度-金属丰度关系
梁艳春1; HAMMER Francois2; 邓李才1; 赵刚1
2007
Source Publication天文学进展
ISSN1000-8349
Volume025Issue:001Pages:22
Abstract金属丰度与星系光度是星系的重要特征参量,研究它们之间的关系有助于理解星系中恒星质量与金属成分的累积过程。评述了星系的光度一金属丰度关系的最新研究进展,包括对近邻星系、中等红移星系(0.4〈Z〈1)及高红移星系(Z〉2)的研究结果。由于观测样本跨越较宽的宇宙学时标,可以由此来探讨这一关系的演化过程,从而帮助理解星系演化的整体图景。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/43678
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.GEPI, Observatoire de Paris-Meudon
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
梁艳春,HAMMER Francois,邓李才,等. 星系金属丰度的研究进展(Ⅱ):光度-金属丰度关系[J]. 天文学进展,2007,025(001):22.
APA 梁艳春,HAMMER Francois,邓李才,&赵刚.(2007).星系金属丰度的研究进展(Ⅱ):光度-金属丰度关系.天文学进展,025(001),22.
MLA 梁艳春,et al."星系金属丰度的研究进展(Ⅱ):光度-金属丰度关系".天文学进展 025.001(2007):22.
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