Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Planet Formation at Cosmic Dawn: Planetesimals in H2O-rich Disks around Low-mass Stars

  • Authors: Eduard I. Vorobyov, Daniel J. Whalen, Muhammad A. Latif, Alexander Skliarevskii, Christopher Jessop, Ryoki Matsukoba, Takashi Hosokawa, Devesh Nandal

Eduard I. Vorobyov et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 6.

Total planetesimal masses for the fiducial model (solid black) and parameter study models. The latter include the models with vfrag = 3.0 m s−1 (solid red), ﹩{\xi }_{{\rm{d2g}}}^{{\rm{init}}}=2\times 1{0}^{-4}﹩ (solid blue), with the streaming instability criteria from R. Li & A. N. Youdin (2021) (dashed green), MRI with solar metallicity excitation criteria (cyan), and gravitoturbulence (pink).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse