NEW LIGHT ON FAINT STARS .6. STRUCTURE AND EVOLUTION OF THE GALACTIC SPHEROID

被引：148

作者：

GILMORE, G ^{[1
]}

机构：

[1] CARNEGIE INST WASHINGTON,MT WILSON & LAS CAMPANAS OBSERV,PASADENA,CA 91101

来源：

关键词：

D O I：

10.1093/mnras/207.2.223

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：223 / 240

页数：18

共 66 条

[1] THE GALACTIC SPHEROID
BAHCALL, JN
SCHMIDT, M
SONEIRA, RM
[J]. ASTROPHYSICAL JOURNAL, 1983, 265 (02) : 730 - 747
[2] PREDICTED STAR COUNTS IN SELECTED FIELDS AND PHOTOMETRIC BANDS - APPLICATIONS TO GALACTIC STRUCTURE, THE DISK LUMINOSITY FUNCTION, AND THE DETECTION OF A MASSIVE HALO
BAHCALL, JN
SONEIRA, RM
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1981, 47 (04) : 357 - &
[3] THE UNIVERSE AT FAINT MAGNITUDES .1. MODELS FOR THE GALAXY AND THE PREDICTED STAR COUNTS
BAHCALL, JN
SONEIRA, RM
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1980, 44 (01) : 73 - 110
[4] BAHCALL JN, 1983, ASTROPHYS J
[5] BECKER W, 1980, ASTRON ASTROPHYS, V87, P80
[6] BECKER W, 1972, ASTRONOMY, P9
[7] BLAAUW A, 1978, ASTRONOMICAL PAPERS, P33
[8] Blaauw A., 1965, GALACTIC STRUCTURE
[9] BROOKS K, 1981, THESIS U CALIFORNIA
[10] BROOKS K, 1979, B AM ASTRON SOC, V11, P43