The Submillimeter Observation Of The Transition Disk System Of Hd135344

Details The Submillimeter Observation Of The Transition Disk System Of Hd135344 The Submillimeter Observation Of The Transition Disk System Of Hd135344

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21360108l&link_type=abstract

American Astronomical Society, AAS Meeting #213, #601.08

Astronomy and Astrophysics

Astronomy

Scientific paper

17 Myr-old HD 135344 has been suggested as the one of the rare transition systems based on its far-infrared excess above the expected photospheric flux level and a clear detection of CO emission. This system was suggested to have a large inner gap, R 45 AU, from the analysis of the spectral energy distribution (SED) covering from optical to sub-mm wavelength. We will present the strong evidence for the inner gap in the dust continuum and 13CO (J=2-1) molecular line maps from the SubMillimeter Array (SMA) observations. This object will be the one of the best targets to be a disk-planet system which is the ideal laboratory to study the planet formation mechanism, if we consider that the inner gap is involved the clear-up process due to the planet formation.

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