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

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An Optimum Supply-Demand Equilibrium?, bands. The observations were performed from Oct to Nov, 1994 at the Siding Spring Observatory. We used a 25 cm/F3.5 Newtonian telescope equipped with a 512x512 PtSi-Camera (Ueno et al. 1992). The plate scale was 4.″6 x 6.″0/pixel and the total field of view was 40.′2 x 52.′3. The system was attache

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Erika Fernández-Gómez,Beatriz Feijoo galaxies. Tidal dwarfs are found far from the interacting parent galaxies, associated with massive clouds of atomic hydrogen located at the tip of long tidal tails. These newly formed galaxies are among the best cases for the study of galaxy formation in the nearby Universe.

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Manukonda Rabindranath,Aradhana Kumari Singhr to accretion and the triggering of star formation, show distinct HI signatures. Interactions and mergers in the recent past can also be recognized in the HI structure and kinematics. Recent 21cm line surveys of large samples of galaxies indicate that at least one out of every four galaxies shows s

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The Changing Face of Capitalism,s during an encounter, and the percentage of HI in the tails increases with the merging stage. However, the opposite is true for the molecular gas, which is observed highly concentrated towards the nuclei of interacting galaxies, amounting to a significant fraction of the dynamical mass. Statistical

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https://doi.org/10.1007/978-94-011-4665-4Galaxy; Universe; active galactic nuclei; astronomy

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