The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud

YNAO OpenIR > 恒星物理研究组

	The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud
	Gong ZG(龚志刚); Li Y(李焱)
会议录名称	Procceedings of IAU Symposia - The Carbon Star Phenomenon
	2000
卷号	177
页码	199-204
DOI	10.1017/S0074180900002412
产权排序	第1完成单位
收录类别	其他
会议名称	the 177th Symposium of the International Astronomical Union
会议日期	1996-05-27
会议地点	Antalya, Turkey
摘要	The evolutionary status and pulsational characteristics of AGB stars in the LMC have been studied. It is found that only those stars with a small mixing-length ratio can fit the observed period-luminosity relation. Strong non-adiabatic effects were found in the outer envelope and must be taken into account in future work.
项目资助者	N/A
语种	英语
学科领域	天文学 ; 天体物理学 ; 恒星与银河系
出版者	Kluwer Academic Publishers
URL	查看原文
归档日期	2000-12-31
引用统计
文献类型	会议论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/267
专题	恒星物理研究组
作者单位	Yunnan Observatory, Kunming, P.R. China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Gong ZG,Li Y. The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud[C]:Kluwer Academic Publishers,2000:199-204.