Planets opening dust gaps in gas disks

Abstract

We investigate the interaction of gas and dust in a protoplanetary disk in the presence of a massive planet using a new two-fluid hydrodynamics code. In view of future observations of planet-forming disks we focus on the condition for gap formation in the dust fluid. While only planets more massive than 1 Jupiter mass (MJ) open up a gap in the gas disk, we find that a planet of 0.1 MJ already creates a gap in the dust disk. This makes it easier to find lower-mass planets orbiting in their protoplanetary disk if there is a significant population of mm-sized particles.

5 pages, 3 figures, accepted for publication in A&A Letters

References in corpus (5)

• Radial Flow of Dust Particles in Accretion Disks
• Mass Flow and Accretion through gaps in Accretion Discs
• Planets opening dust gaps in gas disks
• Dust Migration and Morphology in Optically Thin Circumstellar Gas Disks
• Detecting planets in protoplanetary disks: A prospective study

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