2 research outputs found
Determining the mid-plane conditions of circumstellar discs using gas and dust modelling: a study of HD 163296
The mass of gas in protoplanetary discs is a quantity of great interest for
assessing their planet formation potential. Disc gas masses are, however,
traditionally inferred from measured dust masses by applying an assumed
standard gas-to-dust ratio of . Furthermore, measuring gas masses
based on CO observations has been hindered by the effects of CO freeze-out.
Here we present a novel approach to study the mid-plane gas by combining
CO line modelling, CO snowline observations and the spectral energy
distribution (SED) and selectively study the inner tens of au where freeze-out
is not relevant. We apply the modelling technique to the disc around the Herbig
Ae star HD 163296 with particular focus on the regions within the CO snowline
radius, measured to be at 90 au in this disc. Our models yield the mass of
CO in this inner disc region of
M. We
find that most of our models yield a notably low , especially in the
disc mid-plane (). Our only models with a more interstellar medium
(ISM)-like require CO to be underabundant with respect to the ISM
abundances and a significant depletion of sub-micron grains, which is not
supported by scattered light observations. Our technique can be applied to a
range of discs and opens up a possibility of measuring gas and dust masses in
discs within the CO snowline location without making assumptions about the
gas-to-dust ratio.This work has been supported by the DISCSIM project, grant agreement 341137 funded by the European Research Council under ERC-2013-ADG. DMB is funded by this ERC grant and an STFC studentship. OP is supported by the Royal Society Dorothy Hodgkin Fellowship. During a part of this project OP was supported by the European Union through ERC grant number 279973. TJH is funded by the STFC consolidated grant ST/K000985/1.This is the final version of the article. It first appeared from Oxford University Press via http://dx.doi.org/10.1093/mnras/stw132
Grand Challenges in Protoplanetary Disc Modelling
The Protoplanetary Discussions conference --- held in Edinburgh, UK, from 7th
--11th March 2016 --- included several open sessions led by participants. This
paper reports on the discussions collectively concerned with the multiphysics
modelling of protoplanetary discs, including the self-consistent calculation of
gas and dust dynamics, radiative transfer and chemistry. After a short
introduction to each of these disciplines in isolation, we identify a series of
burning questions and grand challenges associated with their continuing
development and integration. We then discuss potential pathways towards solving
these challenges, grouped by strategical, technical and collaborative
developments. This paper is not intended to be a review, but rather to motivate
and direct future research and collaboration across typically distinct fields
based on \textit{community driven input}, to encourage further progress in our
understanding of circumstellar and protoplanetary discs