Constraining turbulence in protoplanetary discs using the gap contrast: an application to the DSHARP sample
E. Pizzati, G. P. Rosotti, B. Tabone

TL;DR
This study estimates turbulence levels in protoplanetary discs by analyzing gap contrast differences in DSHARP observations, finding generally low turbulence and providing criteria for selecting suitable discs for such measurements.
Contribution
It introduces a novel indirect method to constrain dust scale heights and turbulence levels in protoplanetary discs using gap contrast asymmetries in ALMA data.
Findings
Most discs have low dust scale heights ($ extless$4 AU at 100 AU)
Turbulence levels are constrained to $ extless$10^{-3}-10^{-4}$ in most cases
Method is limited by disc inclination and gap depth in some systems
Abstract
Constraining the strength of gas turbulence in protoplanetary discs is an open problem that has relevant implications for the physics of gas accretion and planet formation. In this work, we gauge the amount of turbulence in 6 of the discs observed in the DSHARP programme by indirectly measuring the vertical distribution of their dust component. We employ the differences in the gap contrasts observed along the major and the minor axes due to projection effects, and build a radiative transfer model to reproduce these features for different values of the dust scale heights. We find that (a) the scale heights that yield a better agreement with data are generally low ( AU at a radial distance of AU), and in almost all cases we are only able to place upper limits on their exact values; these conclusions imply (assuming an average Stokes number of ) low…
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