骗子
发表于 2025-3-23 09:49:24
Ilan Fridental,Yaron Finkelsteinterized by different galactic orbits. (1) OH/IR stars in the galactic disk on almost circular orbits; (2) OH/IR stars in the galactic bulge on orbits of lower angular momentum; (3) OH/IR stars within 150 pc from the galactic center forming a rapidly rotating system.
Conserve
发表于 2025-3-23 16:40:21
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craving
发表于 2025-3-23 20:20:29
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ingenue
发表于 2025-3-23 23:16:37
Trends in Digital Image Processing Researche dwarf ellipticals of the similar mass (the biased wind). Unfortunately, the observational data available at present of stellar populations of the bulges are not yet sufficient to get a firm conclusion on the origin of the bulges.
滑稽
发表于 2025-3-24 04:53:34
N. D. Gunn,J. Byrne,E. B. Holubthan halo properties alone. This is clearest for systems with low B/D ratio, where bulge velocity dispersions are similar to disk velocity dispersions. Constraints on the stellar formation scenarios are discussed.
异常
发表于 2025-3-24 10:25:53
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单调性
发表于 2025-3-24 11:56:55
Stellar Population Synthesise dwarf ellipticals of the similar mass (the biased wind). Unfortunately, the observational data available at present of stellar populations of the bulges are not yet sufficient to get a firm conclusion on the origin of the bulges.
Tincture
发表于 2025-3-24 15:36:31
What is the Connection between Ellipticals and Bulges ?than halo properties alone. This is clearest for systems with low B/D ratio, where bulge velocity dispersions are similar to disk velocity dispersions. Constraints on the stellar formation scenarios are discussed.
事先无准备
发表于 2025-3-24 19:26:22
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obsolete
发表于 2025-3-25 00:53:18
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