Angular Momentum Transfer due to Galactic Winds and Cooling Flows

V. Missoulis

doi:10.1007/978-94-011-4665-4_49

Galaxy Interactions at Low and High Redshift pp 201-201 | Cite as

Angular Momentum Transfer due to Galactic Winds and Cooling Flows

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V. Missoulis

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Part of the International Astronomical Union book series (IAUS, volume 186)

Abstract

We examine a model of galaxy formation where the bulge is formed at very early stages and this burst of star formation leads to a galactic wind which interacts with a huge surrounding gaseous envelope.

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References

Missoulis, V. 1994, Astron. Reports, 38, 12ADSGoogle Scholar

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Authors and Affiliations

V. Missoulis
- 1

1.Astronomical InstituteNational Observatory of AthensAthensGreece

About this paper

Cite this paper as:: Missoulis V. (1999) Angular Momentum Transfer due to Galactic Winds and Cooling Flows. In: Barnes J.E., Sanders D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht

DOI https://doi.org/10.1007/978-94-011-4665-4_49
Publisher Name Springer, Dordrecht
Print ISBN 978-0-7923-5833-6
Online ISBN 978-94-011-4665-4
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