Titlebook: Galaxy Interactions at Low and High Redshift; Proceedings of the 1 J. E. Barnes,D. B. Sanders Conference proceedings 1999 Springer Science+

分類

書目名稱Galaxy Interactions at Low and High Redshift影響因子(影響力)




書目名稱Galaxy Interactions at Low and High Redshift影響因子(影響力)學(xué)科排名




書目名稱Galaxy Interactions at Low and High Redshift網(wǎng)絡(luò)公開度




書目名稱Galaxy Interactions at Low and High Redshift網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Galaxy Interactions at Low and High Redshift被引頻次




書目名稱Galaxy Interactions at Low and High Redshift被引頻次學(xué)科排名




書目名稱Galaxy Interactions at Low and High Redshift年度引用




書目名稱Galaxy Interactions at Low and High Redshift年度引用學(xué)科排名




書目名稱Galaxy Interactions at Low and High Redshift讀者反饋




書目名稱Galaxy Interactions at Low and High Redshift讀者反饋學(xué)科排名

不遵守

無關(guān)緊要

What can we Learn From the Local Group About the Role of Interactions in Galaxy Formation,the role of interactions in galaxy formation. Bulges are potentially of particular interest for galaxy formation because they are widely suspected to be the seeds for galaxy formation. Sites of active star formation at high redshift are often regarded as spheroids in the process of formation. In thi

修飾

The Magellanic Stream and The Magellanic Cloud System,eproduced the Magellanic Stream (Murai and Fujimoto 1980; Lin and Lynden-Bell 1982; Gardiner et al. 1994; Gardiner and Noguchi 1995; Lin et al. 1995), a narrow band of diffuse atomic hydrogen gas emerging from the SMC region, passing by the South Galactic Pole along an overhead great circle spanning

口味

The Nature and Fate of the Sagittarius Dwarf Galaxy,d into the Milky Way. This unique event allows the physics of galactic merging to be probed in unprecedented detail, and may shed light on the hypothesized population of primordial galaxies that merged to form the Milky Way.

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呼吸

The Magellanic Stream Revisited,s in accordance with the Keplerian law at the distance of 50 kpc, while others have come to consider that the rotation curve of the Milky Way, essentially stays flat or is still increasing at the distance of the Magellanic Clouds and the Magellanic Stream.

Prosaic

Are the Bulge C-Stars Related to the Sagittarius Dwarf Galaxy?,, are ideal tracers for such an event. Ng & Schultheis (1997) suggested that the Bulge carbon stars (Azzopardi et al. 1991; ALRW) might be at SDG’s distance. In the galactic Bulge these stars are completely different from carbon stars found in the LMC, SMC and dwarf spheroidal galaxies. If one keeps

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