作者: T. Henning , W. Kley , S. Wolf , F. Gueth
DOI: 10.1086/339544
关键词:
摘要: We investigate the possibility of finding evidence for planets in circumstellar disks by infrared and submillimeter interferometry. present simulations a disk around solar-type star with an embedded planet 1 Jupiter mass. The three-dimensional density structure results from hydrodynamical simulations. On basis radiative transfer simulations, images this system were calculated. intensity maps provide simulation Very Large Telescope Interferometer (VLTI; equipped mid-infrared instrument MIDI) Atacama Millimeter Array (ALMA). While MIDI/VLTI will not to distinguish between or without gap on visibility measurements, ALMA necessary direct detection.