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Titlebook: Galactic Bulges; Proceedings of the 1 Herwig Dejonghe,Harm J. Habing Conference proceedings 1993 Kluwer Academic Publishers 1993 Bulge.Gala

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11#
發(fā)表于 2025-3-23 09:49:24 | 只看該作者
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.
12#
發(fā)表于 2025-3-23 16:40:21 | 只看該作者
13#
發(fā)表于 2025-3-23 20:20:29 | 只看該作者
14#
發(fā)表于 2025-3-23 23:16:37 | 只看該作者
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.
15#
發(fā)表于 2025-3-24 04:53:34 | 只看該作者
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.
16#
發(fā)表于 2025-3-24 10:25:53 | 只看該作者
17#
發(fā)表于 2025-3-24 11:56:55 | 只看該作者
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.
18#
發(fā)表于 2025-3-24 15:36:31 | 只看該作者
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.
19#
發(fā)表于 2025-3-24 19:26:22 | 只看該作者
20#
發(fā)表于 2025-3-25 00:53:18 | 只看該作者
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