1 code implementation • 29 Apr 2017 • D. Macdonald, Orsola De Marco, Eric Lagadec, Jun Ma, O. Chesneau
Our result is consistent with a large dusty disc with similar parameter values to those previously found by Chesneau et al., except for a larger dust mass of $3. 5^{+7. 5}_{-2. 2}\times10^{-5}$ M$_{\odot}$.
Solar and Stellar Astrophysics