RATE OF STAR FORMATION IN M31 AND LARGE MAGELLANIC CLOUD

被引：0

作者：

TOSA, M ^{[1
]}

HAMAJIMA, K ^{[1
]}

机构：

[1] NAGOYA UNIV,DEPT PHYS,NAGOYA,JAPAN

来源：

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：501 / 505

页数：5

共 14 条

[1] POSITIONS OF EMISSION NEBULAE IN M31
BAADE, W
ARP, H
[J]. ASTROPHYSICAL JOURNAL, 1964, 139 (04) : 1027 - &
[2] EINASTO J, 1972, ASTROPHYS LETT COMM, V11, P195
[3] Einasto J., 1970, Spiral structure of our galaxy, P42
[4] GUIBERT J, 1974, ASTRON ASTROPHYS, V30, P353
[5] RATE OF STAR FORMATION IN M31
HARTWICK, FD
[J]. ASTROPHYSICAL JOURNAL, 1971, 163 (02) : 431 - &
[6] Henize K. G., 1956, AP J S, V2, P315
[7] Lindsay E. M., 1963, IRISH ASTRON J, V6, P51
[8] MCGEE RX, 1964, GALAXY MAGELLANIC CL, P289
[9] A HIGH-RESOLUTION 21-CM HYDROGEN-LINE SURVEY OF ANDROMEDA NEBULA
ROBERTS, MS
[J]. ASTROPHYSICAL JOURNAL, 1966, 144 (02) : 639 - &
[10] Rubin V. C., 1970, Spiral structure of our galaxy, P61