CARBON STARS IN THE GLOBULAR-CLUSTERS OF THE MAGELLANIC CLOUDS

被引:76
|
作者
MOULD, J
AARONSON, M
机构
[1] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85721
[2] CARNEGIE INST WASHINGTON,HALE OBSERV,PASADENA,CA 91101
来源
ASTROPHYSICAL JOURNAL | 1979年 / 232卷 / 02期
关键词
D O I
10.1086/157302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:421 / 427
页数:7
相关论文
共 50 条
  • [21] HIGH-RESOLUTION SPECTROSCOPY OF NEAR MAIN-SEQUENCE B-STARS OF BLUE GLOBULAR-CLUSTERS IN THE MAGELLANIC CLOUDS
    JUTTNER, A
    REITERMANN, A
    STAHL, O
    WOLF, B
    ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1989, 81 (01): : 93 - 102
  • [22] DUST CLOUDS WITHIN GLOBULAR-CLUSTERS - POLARIZATION
    FORTE, JC
    MENDEZ, M
    ASTROPHYSICAL JOURNAL, 1989, 345 (01): : 222 - 229
  • [23] MASSES OF SOME GLOBULAR CLUSTERS IN MAGELLANIC CLOUDS
    CHUN, MS
    ASTRONOMICAL JOURNAL, 1978, 83 (09): : 1062 - 1069
  • [24] BE STARS IN YOUNG CLUSTERS IN THE MAGELLANIC CLOUDS
    GREBEL, EK
    ROBERTS, WJ
    WILL, JM
    DEBOER, KS
    SPACE SCIENCE REVIEWS, 1993, 66 (1-4) : 65 - 68
  • [25] COMPARISON OF GLOBULAR CLUSTERS IN THE GALAXY AND IN THE MAGELLANIC CLOUDS
    THACKERAY, AD
    ASTRONOMICAL JOURNAL, 1959, 64 (10): : 437 - 441
  • [26] ISO observations of the Magellanic Clouds globular clusters
    Tanabé, T
    Nishida, S
    Nakada, Y
    Onaka, T
    Glass, IS
    Sauvage, M
    UNIVERSE AS SEEN BY ISO, VOLS I AND II, 1999, 427 : 409 - 411
  • [27] SEARCH FOR VARIABLE-STARS IN GLOBULAR-CLUSTERS
    HAZENLILLER, ML
    IAU SYMPOSIA, 1986, (118): : 287 - 288
  • [28] THE CHEMICAL-COMPOSITION OF STARS IN GLOBULAR-CLUSTERS
    PILACHOWSKI, CA
    SNEDEN, C
    WALLERSTEIN, G
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1983, 52 (03): : 241 - 287
  • [29] Systematic study of AGB stars in the intermediate-age globular clusters in the Magellanic Clouds
    Tanabé, T
    Nishida, S
    Nakada, Y
    Onaka, T
    Glass, IS
    Sauvage, M
    ASYMPTOTIC GIANT BRANCH STARS, 1999, (191): : 573 - 578
  • [30] M AND S STARS IN LMC GLOBULAR-CLUSTERS
    EVANS, TL
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1984, 208 (02) : 447 - 458