THE DISTRIBUTION OF HORIZONTAL BRANCH STARS IN THE GLOBULAR CLUSTER-M 3

被引:2
|
作者
WOOLF, NJ
机构
关键词
D O I
10.1086/127704
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:339 / 339
页数:1
相关论文
共 50 条
  • [21] Rotation of horizontal-branch stars in globular clusters
    Sills, A
    Pinsonneault, MH
    ASTROPHYSICAL JOURNAL, 2000, 540 (01): : 489 - 503
  • [22] APPLICATION OF THE INFRARED FLUX METHOD TO GLOBULAR-CLUSTER STARS - THE M3 GIANT BRANCH
    ARRIBAS, S
    ROGER, CM
    ASTRONOMY & ASTROPHYSICS, 1987, 178 (1-2) : 106 - 113
  • [23] CONSTRAINTS ON HELIUM ENHANCEMENT IN THE GLOBULAR CLUSTER M3 (NGC 5272): THE HORIZONTAL BRANCH TEST
    Catelan, M.
    Grundahl, F.
    Sweigart, A. V.
    Valcarce, A. A. R.
    Cortes, C.
    ASTROPHYSICAL JOURNAL LETTERS, 2009, 695 (01) : L97 - L102
  • [24] RATIO OF HORIZONTAL BRANCH STARS TO RED GIANT STARS IN GLOBULAR CLUSTERS
    IBEN, I
    ROOD, RT
    STROM, KM
    STROM, SE
    NATURE, 1969, 224 (5223) : 1006 - &
  • [25] UV photometry of spotted stars in the horizontal branch of the globular cluster NGC 2808 using AstroSat
    Prabhu, Deepthi S.
    Subramaniam, Annapurni
    Sahu, Snehalata
    JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 2021, 42 (02)
  • [26] The variable stars and blue horizontal branch of the metal-rich globular cluster NGC 6441
    Layden, AC
    Ritter, LA
    Welch, DL
    Webb, TMA
    ASTRONOMICAL JOURNAL, 1999, 117 (03): : 1313 - 1331
  • [27] SPECTRA OF BLUE HORIZONTAL-BRANCH STARS IN 3 NORTHERN GLOBULAR CLUSTERS
    SARGENT, WLW
    ASTROPHYSICAL JOURNAL, 1967, 148 (3P2): : L147 - &
  • [28] DENSITY DISTRIBUTION OF BRIGHT STARS IN GLOBULAR CLUSTER M56
    KHOLOPOV, PN
    SOVIET ASTRONOMY AJ USSR, 1971, 15 (02): : 247 - &
  • [29] THE EFFECT OF THE HORIZONTAL BRANCH ON GLOBULAR-CLUSTER COLORS
    SILCHENKO, OK
    SOVIET ASTRONOMY LETTERS, 1983, 9 (03): : 145 - 148
  • [30] On the horizontal branch of the galactic globular cluster NGC 2808
    Castellani, V
    Iannicola, G
    Bono, G
    Zoccali, M
    Cassisi, S
    Buonanno, R
    ASTRONOMY & ASTROPHYSICS, 2006, 446 (02): : 569 - 577