Angular momentum transport at early times

Details Angular momentum transport at early times Angular momentum transport at early times

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..dppjm4001z&link_type=abstract

American Physical Society, 49th Annual Meeting of the Division of Plasma Physics, November 12-16, 2007, abstract #JM4.001

Physics

Plasma Physics

Scientific paper

It is well known that angular momentum must be efficiently removed from interstellar clouds as they contract and eventually collapse to form stars. At the present epoch, angular momentum is transported primarily by magnetic fields. At the time the first stars formed, galactic magnetic fields were probably either absent or were much weaker than they are now. I will discuss the growth of magnetic fields in star forming regions and their role in angular momentum transport under primordial conditions.

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