名词
发表于 2025-3-28 15:48:40
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.
常到
发表于 2025-3-28 20:14:39
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转折点
发表于 2025-3-28 23:42:40
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.
cognizant
发表于 2025-3-29 03:52:08
Malcolm S. LongairExcellently suited as a textbook
中和
发表于 2025-3-29 08:38:59
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相互影响
发表于 2025-3-29 14:20:37
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
Frequency
发表于 2025-3-29 18:29:37
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
谈判
发表于 2025-3-29 22:04:44
K. Schmid,H. Fürer,G. Dändlikertures 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
施魔法
发表于 2025-3-30 01:48:42
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
Malcontent
发表于 2025-3-30 07:38:44
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