CORRELATION BETWEEN M-L AND COLOR FOR SPIRAL GALAXIES

被引：13

作者：

SARGENT, WLW

TINSLEY, BM

机构：

[1] HALE OBSERV,PASADENA,CA 91100

[2] UNIV TEXAS,DALLAS,TX 75222

[3] UNIV TEXAS,AUSTIN,TX 78712

来源：

关键词：

D O I：

10.1093/mnras/168.1.19P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：P19 / P22

页数：4

共 13 条

[1] BALDWIN JR, 1973, ASTROPHYS LETT COMM, V14, P1
[2] DIRACS COSMOLOGICAL COINCIDENCE - EXPLANATION
CLUTTONB.M
[J]. ASTROPHYSICS AND SPACE SCIENCE, 1974, 30 (01) : L1 - L3
[3] ROTATION CURVE AND MASS DISTRIBUTION IN M3I
EMERSON, DT
BALDWIN, JE
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 165 (01) : P9 - P13
[4] FABER SM, 1972, ASTRON ASTROPHYS, V20, P361
[5] LARSON RL, IN PRESS
[6] ANGULAR-MOMENTUM OF SPIRAL GALAXIES .2. DETAILED MODELS AND CORRELATIONS FOR 17 GALAXIES
NORDSIECK, KH
[J]. ASTROPHYSICAL JOURNAL, 1973, 184 (03) : 735 - +
[7] ROSE WK, 1974, PREPRINT
[8] SARGENT WLW, 1973, INT C SUPERNOVAE
[9] HISTORY OF STAR FORMATION AND COLORS OF LATE-TYPE GALAXIES
SEARLE, L
SARGENT, WLW
BAGNUOLO, WG
[J]. ASTROPHYSICAL JOURNAL, 1973, 179 (02) : 427 - 438
[10] TINSLEY BM, 1972, ASTRON ASTROPHYS, V20, P383