Image Details

Choose export citation format:

Diverse Protoplanetary Disk Morphology Produced by a Jupiter-mass Planet

  • Authors: Jaehan Bae, Paola Pinilla, and Tilman Birnstiel

2018 The Astrophysical Journal Letters 864 L26.

  • Provider: AAS Journals

Caption: Figure 5.

Radial distributions of the gas surface density (gray dashed curves, left y-axis) and the continuum opacity at 230 GHz (black solid curves, right y-axis) for (a) Model 1, (b) Model 2, and (c) Model 3. The vertical dotted lines indicate the radial locations where the total grain surface density has a local maximum. Note the radial variations of the continuum opacity across the disks. We adopt the optical constants from Ricci et al. (2010) to calculate the grain opacity.

Other Images in This Article
Copyright and Terms & Conditions