Author of the publication

A radiation hydrodynamics scheme on adaptive meshes using the Variable Eddington Tensor (VET) closure

, , , , , and . (2022)cite arxiv:2203.12177Comment: 7 pages, 2 figures, to appear in the proceedings of IAUS362: The predictive power of computational astrophysics as discovery tool (D. Bisikalo, T. Hanawa, C. Boily, J. Stone, eds.). arXiv admin note: substantial text overlap with arXiv:2202.08778.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

 

Other publications of authors with the same name

Hybrid Adaptive Ray-Moment Method (HARM$^2$): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids, , , , and . (2016)cite arxiv:1607.01802Comment: 27 pages, 8 figures, submitted to Journal of Computational Physics. Referee comments received and will be addressed in final version.Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies II: The Effects of Star Formation Feedback, , and . (2016)cite arxiv:1605.00646Comment: 16 pages, 13 figures. Resubmitted to the Astrophysical Journal after responding to referee comments. 6 TB of simulation data and processed derived data are available at http://dx.doi.org/10.13012/J85Q4T1T. An interactive data exploration widget is available at https://demo.use.yt (click "galaxy_visualization.ipynb"; once the Jupyter notebook launches, click "Cell -> Run All").The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function, , and . (Oct 16, 2015)Star Formation in Atomic Gas. (2012)cite arxiv:1208.1504Comment: 9 pages, 8 figures, submitted to ApJ.The Star Formation Law in Molecule-Poor Galaxies. (2013)cite arxiv:1309.5100Comment: 18 pages, 9 figures, accepted for publication in MNRAS.The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function. (2014)cite arxiv:1402.0867Comment: 88 pages, 19 figures, review article in press for Physics Reports.SLUG - Stochastically Lighting Up Galaxies. II: Quantifying the Effects of Stochasticity on Star Formation Rate Indicators, , and . (2014)cite arxiv:1403.4605Comment: 13 pages, 8 figures. Submitted to MNRAS. Comments are welcome.The Global Evolution of Giant Molecular Clouds II: The Role of Accretion, , , and . (2011)cite arxiv:1105.6097 Comment: 23 Pages, 9 Figures. Resubmitted to ApJ with referee comments. Comments are welcome.Evolution of Blister-Type HII Regions in a Magnetized Medium, and . (2011)cite arxiv:1110.4645 Comment: 15 pages, 17 figures, 1 table.Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters II. The Initial Mass Function from Winds, Turbulence, and Radiation, , and . (2012)cite arxiv:1203.2620Comment: 17 pages, 15 figures, emulateapj format, submitted to ApJ. For movies of the results, see http://www.ucolick.org/~krumholz/downloads.html.