1481291
doi
10.5281/zenodo.1481291
oai:zenodo.org:1481291
Angular Momentum – Conference Summary
Combes, Francoise
Observatoire de Paris, LERMA, College de France, CNRS, PSL Univ., Sorbonne Univ., F-75014, Paris, France
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<p>Angular momentum (AM) is a key parameter to understand galaxy formation and evolution. AM originates in tidal torques between proto-structures at turn around, and from this the specific AM is expected to scale as a power-law of slope 2/3 with mass. However, subsequent evolution re-shuffles this through matter accretion from filaments, mergers, star formation and feedback, secular evolution and AM exchange between baryons and dark matter. Outer parts of galaxies are essential to study since they retain most of the AM and the diagnostics of the evolution. Galaxy IFU surveys have recently provided a wealth of kinematical information in the local universe. In the future, we can expect more statistics in the outer parts, and evolution at high z, including atomic gas with SKA.</p>
Zenodo
2018-11-09
info:eu-repo/semantics/conferencePaper
1481284
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493826
md5:a4652f2b53251b1d78a5f7ad96dd31de
https://zenodo.org/records/1481291/files/combes.pdf
public
10.5281/zenodo.1481284
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doi