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A high-performance and portable asymptotic preserving radiation hydrodynamics code with the M1 model

, , , , and . (2020)cite arxiv:2011.13926.

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3D simulations of globules and pillars formation around HII regions: turbulence and shock curvature, , , , and . (2012)cite arxiv:1207.6400Comment: accepted for publication in A&A.A high-performance and portable asymptotic preserving radiation hydrodynamics code with the M1 model, , , , and . (2020)cite arxiv:2011.13926.Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane, , , , , , , , , and 28 other author(s). (2017)cite arxiv:1705.09877Comment: 15 pages, 12 figures. Accepted for publication by Astronomy and Astrophysics.StarBench: The D-type expansion of an HII region, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1507.05621Comment: 20 pages, 12 Figures, 4 Tables. Accepted for publication in MNRAS. Comments are welcome. Participation in future StarBench tests is also welcome.Age, size, and position of H ii regions in the Galaxy. Expansion of ionized gas in turbulent molecular clouds, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1406.1801Comment: Accepted in A&A.