Data

Radiative transfer model of the IM Lupi protoplanetary disc with a 0, 2, 3, 5 and 7 Jupiter-mass planet, post-processed from the hydrodynamical simulations. As published in Verrios et al. (2022).

Monash University
Christophe Pinte (Aggregated by) Daniel Price (Aggregated by) Josh Calcino (Aggregated by)
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.26180/20145620.v3&rft.title=Radiative transfer model of the IM Lupi protoplanetary disc with a 0, 2, 3, 5 and 7 Jupiter-mass planet, post-processed from the hydrodynamical simulations. As published in Verrios et al. (2022).&rft.identifier=https://doi.org/10.26180/20145620.v3&rft.publisher=Monash University&rft.description=Contains synthetic images of IM Lupi protoplanetary disc at wavelengths of 1.6 microns (data_1.6/RT.fits.gz), 1.25 mm (data_1250/RT.fits.gz) and a datacube of the synthetic 12CO 2-1 line emission from each hydrodynamical model. The directory for each planet mass also contains the parameter files used to setup and perform the simulation (using the phantom smoothed particle hydrodynamics code: https://github.com/danieljprice/phantom) and to perform the radiative transfer, using the MCFOST code (https://github.com/cpinte/mcfost). The figures in the paper were plotted from the cubes using pymcfost (https://github.com/cpinte/pymcfost). The python scripts for these are provided also.&rft.creator=Christophe Pinte&rft.creator=Daniel Price&rft.creator=Josh Calcino&rft.date=2022&rft_rights=CC-BY-4.0&rft_subject=protoplanetary disk&rft_subject=astronomy&rft_subject=IM Lupi&rft_subject=MCFOST&rft_subject=phantom&rft.type=dataset&rft.language=English Access the data
Cite Saved to MyRDA Save to MyRDA

Licence & Rights:

Open Licence view details
CC-BY

CC-BY-4.0

Full description

Contains synthetic images of IM Lupi protoplanetary disc at wavelengths of 1.6 microns (data_1.6/RT.fits.gz), 1.25 mm (data_1250/RT.fits.gz) and a datacube of the synthetic 12CO 2-1 line emission from each hydrodynamical model. The directory for each planet mass also contains the parameter files used to setup and perform the simulation (using the phantom smoothed particle hydrodynamics code: https://github.com/danieljprice/phantom) and to perform the radiative transfer, using the MCFOST code (https://github.com/cpinte/mcfost). The figures in the paper were plotted from the cubes using pymcfost (https://github.com/cpinte/pymcfost). The python scripts for these are provided also.

Issued: 2022-06-24

Created: 2022-07-06

This dataset is part of a larger collection

Click to explore relationships graph
Help

Related People

Subjects
IM Lupi | MCFOST | astronomy | phantom | protoplanetary disk |

User Contributed Tags    

Login to tag this record with meaningful keywords to make it easier to discover

Identifiers
ACN 633 798 857