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Titlebook: Galaxy Formation; Malcolm S. Longair Textbook 19981st edition The Editor(s) (if applicable) and The Author(s), under exclusive license to

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樓主: genial
41#
發(fā)表于 2025-3-28 15:48:40 | 只看該作者
Eva B. Griepp,Randall B. GrieppLet us recall the reasons for taking dark matter, and in particular non-baryonic dark matter, very seriously in the context of galaxy formation.
42#
發(fā)表于 2025-3-28 20:14:39 | 只看該作者
43#
發(fā)表于 2025-3-28 23:42:40 | 只看該作者
Dark Matter and Galaxy FormationLet us recall the reasons for taking dark matter, and in particular non-baryonic dark matter, very seriously in the context of galaxy formation.
44#
發(fā)表于 2025-3-29 03:52:08 | 只看該作者
Malcolm S. LongairExcellently suited as a textbook
45#
發(fā)表于 2025-3-29 08:38:59 | 只看該作者
46#
發(fā)表于 2025-3-29 14:20:37 | 只看該作者
Norsiah Kadir,Mohd Zaini Abd Karimobservation. In this chapter, we concentrate upon the large-scale distribution of matter and radiation in the Universe and deal with galaxies and clusters of galaxies in Chaps. 3 and 4 respectively. The observations described in this chapter provide much of the essential underpinning of modern cosmo
47#
發(fā)表于 2025-3-29 18:29:37 | 只看該作者
Stephanie Ling Jie Lee,Sijie LinUnfortunately, the astrophysics of normal galaxies is only partially under?stood and many important questions remain unresolved. Part of the problem arises from the fact that galaxies are complex, many-body systems. Typically, a galaxy consists of hundreds of millions or billions of stars, it can co
48#
發(fā)表于 2025-3-29 22:04:44 | 只看該作者
K. Schmid,H. Fürer,G. D?ndlikertures on scales much greater than clusters, the vast ‘walls’ which surround the large voids seen in Fig. 2.5. Very few galaxies can be considered to be truly isolated. Rich clusters of galaxies are of particular interest because they are the largest gravitationally bound systems we know of in the Un
49#
發(fā)表于 2025-3-30 01:48:42 | 只看該作者
M. A. Muhs,E. L. Bastin,B. E. Gordont the Universe is isotropic, homogeneous and expanding uniformly at the present epoch. In other words, we smooth out all the finescale structure in the Universe. It is intriguing that this is precisely what Einstein assumed in his static model of 1917, the first fully selfconsistent model of the Uni
50#
發(fā)表于 2025-3-30 07:38:44 | 只看該作者
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