Super-Earths in the TW Hya disc

Research output: Contribution to journalArticleResearchpeer-review

6 Citations (Scopus)

Abstract

We test the hypothesis that the sub-millimetre thermal emission and scattered light gaps seen in recent observations of TW Hya are caused by planet-disc interactions. We perform global three-dimensional dusty smoothed particle hydrodynamics simulations, comparing synthetic observations of our models with dust thermal emission, CO emission, and scattered light observations. We find that the dust gaps observed at 24 au and 41 au can be explained by two super-Earths (∼4 Ma). A planet of approximately Saturn-mass can explain the CO emission and the depth and width of the gap seen in scattered light at 94 au. Our model produces a prominent spiral arm while there are only hints of this in the data. To avoid runaway growth and migration of the planets we require a disc mass of lesssim 10-2, mathrm M o in agreement with CO observations but 10-100 times lower than the estimate from HD line emission.

Original languageEnglish
Pages (from-to)L130-L135
Number of pages6
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume484
Issue number1
DOIs
Publication statusPublished - 1 Mar 2019

Keywords

  • hydrodynamics
  • infrared: planetary systems
  • planet-disc interactions
  • protoplanetary discs
  • stars: individual (TW Hydrae)
  • submillimetre: planetary systems

Cite this