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

Ordeal

Needlework

注入

A Near Infrared Survey of the LMC, 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

天真

Soliloquy

楓樹

Cervical-Spine

SNEER

Extended Gas in Interacting Systems,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

財(cái)政

https://doi.org/10.1007/978-1-4612-0387-2 Observations of interacting galaxies at low redshifts (. ? 0.2) yield detailed information about many of the processes at work. I briefly review these processes and the growing evidence that mergers play a major role in the delayed formation of elliptical and early-type disk galaxies both in the fi

Pulmonary-Veins