Turbulence In Tw Hya: Methods And Limitations
Abstract
I will present recent ALMA observations of a depression in CS and CN radial emission around TW Hya, which are co-spatial with a well known dip in scattered light emission. I will discuss the utility of molecular tracers in determining the physical and kinematical conditions around such a features with a view to connect what we observe in scattered light to deeper in the protoplanetary disk.
- Publication:
-
Resolving planet formation in the era of ALMA and extreme AO. Proceedings of the conference held 16-20 May
- Pub Date:
- July 2016
- DOI:
- 10.5281/zenodo.58212
- Bibcode:
- 2016rpfe.confE..12T
- Keywords:
-
- Zenodo community planet-formation2016