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The Fundamental Physics of Angular Momentum Evolution in a ΛCDM Scenario

Published online by Cambridge University Press:  03 March 2020

Susana Pedrosa
Susana Pedrosa*
Affiliation:
Institute for Astronomy and Space Science, CONICET - UBA, Ciudad Universitaria, Buenos Aires, Argentina email: supe@iafe.uba.ar Dept. de Fsica Teórica, Univ. Autónoma de Madrid Cantoblanco, Madrid, Espana
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Abstract

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Galaxy formation is a very complex process in which many different physical mechanisms intervene. Within the LCDM paradigm processes such as gas inflows and outflows, mergers and interactions contribute to the redistribution of the angular momentum content of the structures. Recent observational results have brought new insights and also triggered several theoretical studies. Some of these new contributions will be analysed here.

Keywords

galaxies: formationgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 222 - 227
Copyright
© International Astronomical Union 2020

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