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Title: Evolution of disk galaxies and the SO problem, revisited

Journal Article · · Astrophys. J., Suppl. Ser.; (United States)
DOI:https://doi.org/10.1086/190819· OSTI ID:7063706

We begin by summerizing the relevant properties of clusters of galaxies in relation to their ability to alter the course of galaxy evolution. Previous work on the effect of environment on the evolution of disk galaxies is also summerized and critiqued. The extensive data base of Bothun is then used to reexamine the issue of the role of the environment in motivating the evolution of disk galaxies. This data base consists of radio and optical observations of approx.350 galaxies in the clusters Peg I, Cancer, Pices, Coma, A1367, Z74--23, Hercules, A539, and A400. The data are portrayed in the color-gas content plane (log M/sub H//L/sub B/ vs. (B--V)/sup T//sub 0/), and theoretical evolutionary tracks have been constructed in that plane to serve as an adjunct to data interpretation. All analysis is done solely on the basis of the measurable quantities themselves, as opposed to morphological considerations. We find that spiral galaxies exhibit such a wide range in their integrated properties that attempting to force then into ''narrow'' morphological bins is neither practical or physically meaningful. With respect to the question of environmental modification of disk galaxies in clusters, we find the great majority of the data to mitigate strongly against any global environmental processes as having been important in determining the particular evolutionary history of cluster galaxies. Our basic conclusion is that initial conditions of formation and variations in star formation histories have been more important than environmental influences in determining the present-day character of spiral galaxies in clusters. The key parameter may well be the amount of neutral hydrogen remaining after star formation in the bulge component has ceased.

Research Organization:
University of Washington and Harvard-Smithsonian Center for Astrophysics
OSTI ID:
7063706
Journal Information:
Astrophys. J., Suppl. Ser.; (United States), Vol. 50:1
Country of Publication:
United States
Language:
English