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Titlebook: Nearly Normal Galaxies; From the Planck Time S. M. Faber Conference proceedings 1987 Springer-Verlag New York Inc. 1987 Accretion.Inflation

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樓主: Coenzyme
41#
發(fā)表于 2025-3-28 17:42:46 | 只看該作者
42#
發(fā)表于 2025-3-28 18:44:25 | 只看該作者
43#
發(fā)表于 2025-3-29 01:24:17 | 只看該作者
44#
發(fā)表于 2025-3-29 03:41:38 | 只看該作者
45#
發(fā)表于 2025-3-29 08:05:35 | 只看該作者
46#
發(fā)表于 2025-3-29 12:53:38 | 只看該作者
Dwarf Galaxies and Dark Matterarticles orbiting our Galaxy, their Galactocentric radial velocities and distances can be used to constrain the distribution of dark matter in the Galactic halo. Although this problem has been investigated several times in the past [1,2,3,4], there are at least two motivations for another look: (i)
47#
發(fā)表于 2025-3-29 18:45:25 | 只看該作者
48#
發(fā)表于 2025-3-29 20:39:03 | 只看該作者
The Stellar Population at the Galactic Centerrmation in other galactic nuclei but also as an example of star formation in a bulge environment. The star formation process in the deep gravitational potential well at the center of a galaxy may well differ from that process in the less extreme circumstances found in a disk.
49#
發(fā)表于 2025-3-30 02:56:31 | 只看該作者
50#
發(fā)表于 2025-3-30 07:38:24 | 只看該作者
Hot Coronae Around Early Type Galaxies the stars of a bright elliptical galaxy would shed ~5×10... of gas. Over the last 25 years, limits on various forms of gas in early type galaxies became increasingly stringent. Models for a galactic wind, like that of MATHEWS and BAKER [2], were developed to explain the absence of gas. However NORM
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