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Detecting Planets within Disks
Published online by Cambridge University Press: 23 September 2016
Abstract
Possible ways to detect extra-solar planets in circumstellar disks using high-angular resolution measurements (imaging) are discussed. Since dust is expected to outshine the planet by scattering of stellar radiation and thermal emission, the most promising approach is to look for characteristic signatures in the circumstellar disk caused by the interaction with the planet.
- Type
- Part 9: The Influence of Planets During Star Formation
- Information
- Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 441 - 448
- Copyright
- Copyright © Astronomical Society of the Pacific 2004