NAOC Open IR
年轻星团光度函数的演化
胡景耀1; 陈文屏2; 高国钧2
1997
Source Publication天体物理学报
ISSN0253-2379
Volume017Issue:004Pages:401
Abstract利用已发表的Trapezium星团和IC348星团的K波段光度函数和作者获得的NGC663I波段的光度函数,将它分别与不同年龄一次形成或分批形成的模型计算结果作了比较,认为Trapezium星团的年龄为5×10^5年,IC348则为4-6×10^6年,且它们的成员星可能是持续产生的,NGC663的年龄据推算在1-3×10^7年之间。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/40347
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.台湾中央大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
胡景耀,陈文屏,高国钧. 年轻星团光度函数的演化[J]. 天体物理学报,1997,017(004):401.
APA 胡景耀,陈文屏,&高国钧.(1997).年轻星团光度函数的演化.天体物理学报,017(004),401.
MLA 胡景耀,et al."年轻星团光度函数的演化".天体物理学报 017.004(1997):401.
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