General Physical Properties of External Galaxies.
General Physical Properties of External Galaxies.
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外部星系的一般物理特性。
DOI：
10.1007/978-3-642-45932-0_8
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发表时间：
1959
影响因子：
4.8
通讯作者：
G. Vaucouleurs
中科院分区：
文献类型：
--
作者：
G. Vaucouleurs
柯蒂斯[A]和哈勃[B]回顾了1935年以前对星系外星系结构和一般物理性质的早期研究。它们的尺寸、光度和质量的数量级是由哈勃[25]和伦德马克[44]在30多年前确定的。在接下来的十年中，对它们的颜色、光谱和动力学的更详细的研究主要在哈佛大学进行。威尔逊、隆德和斯德哥尔摩天文台。沙普利[C]和沃格特[D]总结了战争结束时的主要结果。
The early investigations into the structure and general physical properties of external galaxies up to 1935 have been reviewed by Curtis [A] and by Hubble [B]. The order of magnitude of their dimensions, luminosities and masses was established over thirty years ago by Hubble [25] and by Lundmark [44]. In the following decade more detailed studies of their colours, spectra and dynamics were undertaken principally at the Harvard, Lick, Mt. Wilson, Lund and Stockholm observatories. The main results available at the end of the war have been summarized by Shapley [C] and by Vogt [D].