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From Magnetized Cores to Protoplanetary Disks

Published online by Cambridge University Press:  21 October 2010

Susana Lizano  and
Frank H. Shu
Susana Lizano
Affiliation:
CRyA, UNAM, Apdo. Postal 72-3, 58089 Morelia, Michoacán, México email: s.lizano@crya.unam.mx
Frank H. Shu
Affiliation:
Physics Department, University of California at San Diego, La Jolla, CA 92093, USA email: fshu@physics.ucsd.edu
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Abstract

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We highlight several recent theoretical results that show how magnetic fields, with the magnitudes currently observed in molecular clouds, affect the structure and evolution of dense cores and protoplanetary disks to form stars and planets.

Keywords

magnetic fieldsstars: formationaccretion: accretion disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 440 - 441
Copyright
Copyright © International Astronomical Union 2010

References

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