Multiple Disk Gaps and Rings Generated by a Single Super-Earth

By R. Dong, Shengtai Li, E. Chiang, Hui Li. 2017

133 citations recorded by the source corpus.

UC Berkeley Vice Chancellor for Research; Berkeley Center for Integrative Planetary Science; LANL's LDRD program; CSES project; NSF; NASA

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/09682c5c41226d4fba378b05aee70c7c1f22ddfe

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In Astronomy and Astrophysics

1. T. Birnstiel
2. S. Andrews
3. D. Wilner
4. Simon Bruderer
5. Xue-Ning Bai
6. C. Dullemond
7. Zhaohuan Zhu
8. A. Hughes

In Nuclear and High Energy Physics

1. J. Carpenter
2. Xue-Ning Bai
3. U. Cambridge
4. Simon Bruderer
5. Andrea Isella
6. A. N. Timokhin

Citations in the corpus

• Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region (2018, background): “…by giant planets, then deeper and wider gaps should be more prevalent around solar-mass stars than around stars of lower mass, although this picture would be complicated by any mass dependence in disk properties (e.g., low-mass planets can more easily open gaps in inviscid disks; Dong et al. 2017).”
• ALMA continuum observations of the protoplanetary disk AS 209. Evidence of multiple gaps opened by a single planet (2017, background): “Furthermore, at extremely low viscosity, Dong et al. (2017) and Bae et al. (2017) showed that planets may open multiple dust gaps in inviscid disks, which raises the interesting possibility that the gaps in AS 209 may be opened by a single planet.”
• The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation (2018, background): “Secondary Gaps/Rings Previous simulations have shown that a planet can introduce many gaps/rings in disks having very low viscosities (Zhu et al. 2014; Bae et al. 2017; Dong et al. 2017).”
• The Disk Substructures at High Angular Resolution Project (DSHARP). II. Characteristics of Annular Substructures (2018, background): “…for many candidate protoplanets in disks with substructure, recent works have explored the possibility that these substructures are created instead by lower-mass planets (i.e., super-Earths) in low-viscosity disks (e.g., Duffell & MacFadyen 2013; Zhu et al. 2014; Dong et al. 2017; Bae et al. 2017).”