THE APSIDAL MOTION OF GIANT BINARY STARS

被引:3
作者
MOTZ, L
机构
关键词
D O I
10.1086/145358
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:434 / 444
页数:11
相关论文
共 10 条
[1]  
CHANDRASEKHAR, 1939, INTRO STUDY STELLAR, P447
[2]  
FEINSTEIN, 1941, REV SCI I, V12, P405
[4]  
HEN, 1933, MN, V93, P451
[5]   RED-GIANT MODELS WITH CHEMICAL INHOMOGENEITIES [J].
HEN, L ;
SCHWARZSCHILD, M .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1949, 109 (06) :631-646
[6]   ON THE PHYSICAL AND CHEMICAL COMPOSITION OF THE SUN [J].
KELLER, G .
ASTROPHYSICAL JOURNAL, 1948, 108 (03) :347-353
[7]   The apsidal motion in binary stars built on a point-source convenctive-core model with varying guillotine factor [J].
Motz, L .
ASTROPHYSICAL JOURNAL, 1941, 94 (02) :253-258
[8]   A STELLAR MODEL FOR RED GIANTS OF HIGH CENTRAL TEMPERATURE [J].
RICHARDSON, RS ;
SCHWARZSCHILD, M .
ASTROPHYSICAL JOURNAL, 1948, 108 (03) :373-387
[9]  
STERNE TE, 1939, MN, V99, P455
[10]  
WOOD, 1946, CONTR PRINCETON U OB, V21, P22