MASS OF M31 AS DETERMINED FROM MOTIONS OF ITS GLOBULAR CLUSTERS

被引:25
作者
HARTWICK, FD
SARGENT, WLW
机构
[1] UNIV VICTORIA,VICTORIA,BRITISH COLUMBI,CANADA
[2] HALE OBSERV,PASADENA,CA
关键词
D O I
10.1086/152873
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:283 / 284
页数:2
相关论文
共 11 条
[1]  
CHRISTENSEN C, 1971, THESIS CALIFORNIA I
[2]   Nebulous objects in Messier 31 provisionally identified as globular clusters [J].
Hubble, E .
ASTROPHYSICAL JOURNAL, 1932, 76 (01) :44-69
[3]  
LOHMANN W, 1956, MITT RECHENINST HE A
[4]   NUMERICAL STUDY OF STABILITY OF FLATTENED GALAXIES - CAN COLD GALAXIES SURVIVE [J].
OSTRIKER, JP ;
PEEBLES, PJE .
ASTROPHYSICAL JOURNAL, 1973, 186 (02) :467-480
[5]  
OSTRIKER JP, 1972, B AM ASTRON SOC, V4, P316
[6]  
PEREK L, 1962, ADV ASTRON ASTROPHYS, V1, P165
[7]   ROTATION OF ANDROMEDA NEBULA FROM A SPECTROSCOPIC SURVEY OF EMISSION REGIONS [J].
RUBIN, VC ;
FORD, WK .
ASTROPHYSICAL JOURNAL, 1970, 159 (02) :379-&
[8]   ABSOLUTE MAGNITUDES OF CEPHEIDS .3. AMPLITUDE AS A FUNCTION OF POSITION IN INSTABILITY STRIP - PERIOD-LUMINOSITY-AMPLITUDE RELATION [J].
SANDAGE, A ;
TAMMANN, GA .
ASTROPHYSICAL JOURNAL, 1971, 167 (02) :293-&
[10]  
VETESNIK M, 1962, B ASTRON I CZECH, V13, P218