ON THE PROPER MOTION OF THE MAGELLANIC CLOUDS AND THE HALO MASS OF OUR GALAXY

被引:153
作者
LIN, DNC [1 ]
LYNDENBELL, D [1 ]
机构
[1] THE OBSERV,INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND
关键词
D O I
10.1093/mnras/198.3.707
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:707 / 721
页数:15
相关论文
共 31 条
[1]  
Allen C. W., 1973, ASTROPHYSICAL QUANTI
[2]  
Davies R. D., 1976, Astronomy and Astrophysics Supplement Series, V23, P181
[3]   TIDAL ORIGIN FOR MAGELLANIC STREAM [J].
DAVIES, RD ;
WRIGHT, AE .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1977, 180 (01) :71-88
[4]  
de Vaucouleurs G., 1972, VISTAS ASTRON, V14, P163, DOI [10.1016/0083-6656(72)90026-8, DOI 10.1016/0083-6656(72)90026-8]
[6]   EXTRA-GALACTIC DISTANCE SCALE .2. DISTANCES OF NEAREST GALAXIES FROM PRIMARY INDICATORS [J].
DEVAUCOULEURS, G .
ASTROPHYSICAL JOURNAL, 1978, 223 (03) :730-739
[7]  
ELSASSER H, 1958, Z ASTROPHYS, V45, P25
[8]   ANALYSIS OF RADIAL VELOCITIES OF STARS AND NEBULAE IN THE MAGELLANIC CLOUDS [J].
FEAST, MW ;
THACKERAY, AD ;
WESSELINK, AJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1961, 122 (05) :433-453
[9]  
FEITZINGER JV, 1977, ASTRON ASTROPHYS, V57, P265
[10]  
FUJIMOTO M, 1969, ASTR ASTROPHYS, V61, P199