Searching for giant planets in young circumstellar disks

Details Searching for giant planets in young circumstellar disks Searching for giant planets in young circumstellar disks

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..167w&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

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Protoplanetary Disk, Planet Formation, Giant Planets

Scientific paper

We investigate the possibility to detect giant planets that are still embedded in young circumstellar disks. Based on hydrodynamical models with different stellar, planetary, and disk masses, different evolutionary stages and different radial positions of the planet we analyze the resulting submillimeter appearance of these systems. We find that the influence of the planet on the continuum spectral energy distribution could not be distinguished from that of other disk parameters. However, dust reemission images of the disks show that the hot region in the proximity of a young planet, along with the gap, could indeed be detected and mapped with the Atacama Large Millimeter Array.

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