Abstract
I HAVE considered1 some of the possible implications of infall of intergalactic matter in galaxies, a process which was proposed by Oort2 to explain the 21 cm observations of high velocity hydrogen “clouds” in our Galaxy. It was pointed out that infall of matter may have a number of important consequences for the structure and evolution of galaxies. In this communication I shall consider in more detail one of these possible consequences, namely the effect of continuing infall of matter on the composition of the interstellar medium and the Population I component of a galaxy. I shall show that in the presence of infalling matter the heavy element content of the interstellar material will tend to approach a constant value which is independent of both the infall rate and the early history of the galaxy, and depends only on stellar evolution processes.
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References
Larson, R. B., Nature, 236, 21 (1972).
Oort, J. H., Astron. Astrophys., 7, 381 (1970).
Larson, R. B., Mon. Not. Roy. Astron. Soc., 145, 405 (1969).
McClure, R. D., Astron. J., 74, 50 (1969).
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LARSON, R. Effect of Infalling Matter on the Heavy Element Content of a Galaxy. Nature Physical Science 236, 7–8 (1972). https://doi.org/10.1038/physci236007a0
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DOI: https://doi.org/10.1038/physci236007a0
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