Search Results for author:
Found 4 papers, 2 papers with code
Particle clustering in turbulence: Prediction of spatial and statistical properties with deep learning
The simulation data are used to train a U-Net deep learning model to predict gridded three-dimensional representations of the particle density and velocity fields, given as input the corresponding fluid fields.
PGNets: Planet mass prediction using convolutional neural networks for radio continuum observations of protoplanetary disks
We provide programs for PGNets and the traditional fitting method from Zhang et al. (2018), and discuss each method's advantages and disadvantages.
Particle Dynamics in 3D Self-gravitating Disks II: Strong Gas Accretion and Thin Dust Disks
Observations suggest that protoplanetary disks have moderate accretion rates onto the central young star, especially at early stages (e. g. HL Tau), indicating moderate disk turbulence.
Earth and Planetary Astrophysics
The ALMA Early Science view of FUor/EXor objects. I. Through the looking-glass of V2775 Ori
We report the detection of a marginally resolved circumstellar disc in the ALMA continuum with an integrated flux of $106 \pm 2$ mJy, characteristic radius of $\sim$ 30 au, inclination of $14. 0^{+7. 8}_{-14. 5}$ deg, and is oriented nearly face-on with respect to the plane of the sky.
Solar and Stellar Astrophysics Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
