You may acknowledge this project by citing the associated papers Commer\c{c}on et al. A&A 658, A52 (2022),
Mignon-Risse et al. A&A 652, A69 (2021), and Mignon-Risse et al. A&A 656, A85 (2021).
This work can be cited with bibtex with
@ARTICLE{2022A&A...658A..52C,
author = {{Commer{\c{c}}on}, B. and {Gonz{'a}lez}, M. and {Mignon-Risse}, R. and {Hennebelle}, P. and {Vaytet}, N.},
title = "{Discs and outflows in the early phases of massive star formation: Influence of magnetic fields and ambipolar diffusion}",
journal = {ap},
keywords = {hydrodynamics, magnetohydrodynamics (MHD), radiative transfer, stars: formation, methods: numerical, stars: massive, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = 2022,
month = feb,
volume = {658},
eid = {A52},
pages = {A52},
doi = {10.1051/0004-6361/202037479},
archivePrefix = {arXiv},
eprint = {2109.10580},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...658A..52C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2021A&A...652A..69M,
author = {{Mignon-Risse}, R. and {Gonz{'a}lez}, M. and {Commer{\c{c}}on}, B. and {Rosdahl}, J.},
title = "{Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer. I. Accretion and multiplicity}",
journal = {ap},
keywords = {accretion, accretion disks, stars: formation, magnetohydrodynamics (MHD), turbulence, stars: massive, methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = 2021,
month = aug,
volume = {652},
eid = {A69},
pages = {A69},
doi = {10.1051/0004-6361/202140617},
archivePrefix = {arXiv},
eprint = {2105.14543},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...652A..69M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2021A&A...656A..85M,
author = {{Mignon-Risse}, R. and {Gonz{'a}lez}, M. and {Commer{\c{c}}on}, B.},
title = "{Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer. II. Outflows}",
journal = {ap},
keywords = {stars: formation, stars: massive, stars: protostars, radiative transfer, magnetohydrodynamics (MHD), methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = 2021,
month = dec,
volume = {656},
eid = {A85},
pages = {A85},
doi = {10.1051/0004-6361/202141648},
archivePrefix = {arXiv},
eprint = {2109.11241},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...656A..85M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
This work was supported by the CNRS "Programme National de Physique Stellaire" (PNPS).
The numerical simulations were produced on the CEA machine Alfven (founded by DIM ACAV+) and using HPC resources from GENCI-CINES (Grants 2018-047247, and A0080407247).
The visualisation of RAMSES data has been done with the OSYRIS python package.
