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From Magnetized Cores to Protoplanetary Disks
Published online by Cambridge University Press: 21 October 2010
Abstract
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.
- 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