ON THE DIFFERENCE IN CHEMICAL COMPOSITION BETWEEN HIGH- AND LOW-VELOCITY STARS

被引：26
作者：
SCHWARZSCHILD, M
SPITZER, L
WILDT, R
机构：
来源：
ASTROPHYSICAL JOURNAL | 1951年 / 114卷 / 03期
关键词：
D O I：
10.1086/145479
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：398 / 406
页数：9
相关论文
共 24 条
[1]  
[Anonymous], 1922, ASTROPHYS J, DOI DOI 10.1086/142660
[2]   The resolution of Messier 32, NGC 205, and the central region of the Andromeda nebula [J].
Baade, W .
ASTROPHYSICAL JOURNAL, 1944, 100 (02) :137-146
[3]  
IWANOWSKA W, 1950, SPECTROPHOTOMETRIC S
[4]  
Justi E., 1938, SPEZIFISCHE WARME EN
[5]  
KEENAN, 1948, AJ, V53, P194
[6]   The extension to the supergiants of the cyanogen criterion of stellar luminosity [J].
Keenan, PC .
ASTROPHYSICAL JOURNAL, 1941, 93 (03) :475-482
[7]   The spectra of CH stars [J].
Keenan, PC .
ASTROPHYSICAL JOURNAL, 1942, 96 (01) :101-105
[8]  
MICZAIKA GR, 1950, Z ASTROPHYS, V27, P1
[9]  
MORGAN, 1943, ATLAS STELLAR SPECTR
[10]  
PAYNE C, 1925, STELLAR ATMOSPHERES, P194
123