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High Angular Resolution Studies of Disks-the Millimetre
Published online by Cambridge University Press: 23 September 2016
Abstract
I briefly review progress in high angular resolution observations of disks at millimetre wavelengths, with a focus on dust continuum observations of the disks surrounding low mass pre-main-sequence stars. I summarize the utility of observations at millimetre wavelengths, where dust emission is largely optically thin, and I touch on several recent directions, including imaging surveys using interferometers, testing physical models of disks with resolved observations, and the complexities introduced by stellar multiplicity.
- Type
- Part 8: Disks
- Information
- Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 381 - 388
- Copyright
- Copyright © Astronomical Society of the Pacific 2004