THE FORMATION OF SUNLIKE STARS

被引：43
作者：
LADA, CJ [1 ]
SHU, FH [1 ]
机构：
[1] UNIV CALIF BERKELEY,DEPT ASTRON,BERKELEY,CA 94720
来源：
SCIENCE | 1990年 / 248卷 / 4955期
关键词：
D O I：
10.1126/science.248.4955.564
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
Understanding how stars like the sun formed constitutes one of the principal challenges confronting modern astrophysics. In recent years, advances in observational technology, particularly at infrared and millimeter wave-lengths, have produced an avalanche of critical data and unexpected discoveries about the process of star formation, which is blocked from external view at optical and shorter wavelengths by an obscuring blanket of interstellar dust. Fueled by this new knowledge, a comprehensive empirical picture of stellar genesis is beginning to emerge, laying the foundations for a coherent theory of the birth of sunlike stars.
引用
收藏
页码：564 / 572
页数：9
相关论文
共 96 条
  • [1] ADAMS F, 1987, APJ, V313, P788
  • [2] INFRARED-SPECTRA OF ROTATING PROTOSTARS
    ADAMS, FC
    SHU, FH
    [J]. ASTROPHYSICAL JOURNAL, 1986, 308 (02) : 836 - 853
  • [3] ADAMS FC, 1988, ASTROPHYS J, V326, P826
  • [4] ADAMS FC, IN PRESS ASTROPHYS J
  • [5] [Anonymous], 1962, ADAA, DOI [DOI 10.1016/B978-1-4831-9919-1.50006-6, 10.1016/B978-1-4831-9919-1.50006-6]
  • [6] APPENZELLER I, 1974, ASTRON ASTROPHYS, V30, P423
  • [7] APPENZELLER I, 1984, ASTRON ASTROPHYS, V141, P108
  • [8] HYDROMAGNETIC-WAVES IN MOLECULAR CLOUDS
    ARONS, J
    MAX, CE
    [J]. ASTROPHYSICAL JOURNAL, 1975, 196 (02) : L77 - L81
  • [9] A DETAILED EXAMINATION OF THE KINEMATICS OF ROTATING DARK CLOUDS
    ARQUILLA, R
    GOLDSMITH, PF
    [J]. ASTROPHYSICAL JOURNAL, 1986, 303 (01) : 356 - 374
  • [10] THE HIGH-VELOCITY MOLECULAR FLOWS NEAR YOUNG STELLAR OBJECTS
    BALLY, J
    LADA, CJ
    [J]. ASTROPHYSICAL JOURNAL, 1983, 265 (02) : 824 - 847
12345678910