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Detecting Planets within Disks

Published online by Cambridge University Press:  23 September 2016

S. Wolf
S. Wolf*
Affiliation:
California Institute of Technology, 1201 E California Blvd, Mail code 105-24, Pasadena, CA, 91125, USA; swolf@astro.caltech.edu

Abstract

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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.

Information

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 

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