How the Galaxy keeps its halo

J. Michael Shull

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How the Galaxy keeps its halo

机译：银河如何保持光环

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Over the centuries, our understanding of the Milky Way has undergone a vast evolution, from the substance of mythology, to early astronomical explanations as a diffuse nebula, to the modern view of a rotating disk of stars and gas embedded in a huge Galactic halo. The halo consists of mysterious dark matter (low-mass stars or exotic particles) together with considerable amounts of visible gas. Forming a cocoon around the Milky Way's disk, the halo stabilizes the disk gravitationally, stores its cosmic rays and acts as a reservoir for the stellar and gaseous debris blown out of the disk.

机译：几个世纪以来，我们对银河系的理解发生了巨大的变化，从神话的本质到早期的天文学对弥漫星云的解释，再到现代的恒星和气体旋转盘嵌在巨大的银河光环中的观点。光环由神秘的暗物质（低质量的恒星或奇异的粒子）以及大量的可见气体组成。光晕在银河系的圆盘周围形成茧，使圆盘重力稳定，存储其宇宙射线，并充当从圆盘吹出的恒星和气态碎屑的储存器。

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《Nature》 |1996年第6576期|p.668-669|共2页
作者
J. Michael Shull;
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收录信息美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
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正文语种 eng
中图分类自然科学总论;
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1. Galaxy Halo Masses from Galaxy-Galaxy Lensing* [J] . Gillian Wilson12, Nick Kaiser1, Gerard A. Luppino1, The Astrophysical journal . 2008,第2期

机译：来自Galaxy-Galaxy Lensing的Galaxy Halo Masses *
2. GALAXY HALO FORMATION IN THE ABSENCE OF VIOLENT RELAXATION AND A UNIVERSAL DENSITY PROFILE OF THE HALO CENTER [J] . A. N. Baushev The Astrophysical journal . 2014,第1期

机译：缺乏晕眩晕晕晕环形成的银河晕形成
3. GALAXY HALO FORMATION IN THE ABSENCE OF VIOLENT RELAXATION AND A UNIVERSAL DENSITY PROFILE OF THE HALO CENTER [J] . A. N. Baushev The Astrophysical journal . 2014,第1期

机译：缺乏晕眩晕晕晕环形成的银河晕形成
4. The Milky Way, the Galactic Halo, and the Halos of Galaxies [C] . Ortwin Gerhard International Astronomical Union., Symposium . 2016

机译：银河系，银河晕和星系的晕
5. Modeling Galaxies in Cosmological Simulations: Using Halo Cores to Model Galaxy Distributions in Clusters, and Constructing the Synthetic Galaxy Catalog CosmoDC2 [D] . Korytov, Danila . 2020

机译：宇宙学模拟中的建模星系：使用晕芯在集群中模拟银河系分布，构建合成银河目录Cosmodc2
6. Galaxy formation with BECDM – I. Turbulence and relaxation of idealized haloes [O] . Philip Mocz, Mark Vogelsberger, Victor H. Robles, -1

机译：BECDM形成银河– I.理想晕环的湍流和松弛
7. The Galaxy–Halo Connection in High-redshift Universe: Details and Evolution of Stellar-to-halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields [O] . Shogo Ishikawa, Nobunari Kashikawa, Jun Toshikawa, 2017

机译：高吊桥宇宙中的Galaxy-Halo连接：Lyman Breaks Beep Fields莱曼突破星系的恒星到光环大规模比率的详细信息和演变

How the Galaxy keeps its halo

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