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}


@BOOK{Osterbrock1989,
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@ARTICLE{Koyama2002,
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}

@ARTICLE{Wibking_2018,
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 primaryClass = {astro-ph.GA},
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}

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}

@ARTICLE{berger1989local,
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}

@ARTICLE{berger1991algorithm,
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@article{AMReX_JOSS,
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  publisher = {The Open Journal},
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  adsnote       = {Provided by the SAO/NASA Astrophysics Data System},
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  date-modified = {2021-09-22 16:56:38 +1000},
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}

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}

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}

@ARTICLE{Howell_2003,
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}

@ARTICLE{Skinner_2019,
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        title = "{FORNAX: A Flexible Code for Multiphysics Astrophysical Simulations}",
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}

@ARTICLE{Skinner_2013,
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}

@ARTICLE{Lowrie_2008,
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}

@ARTICLE{Shu_1989,
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}

@ARTICLE{Quirk_1994,
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}

@ARTICLE{Jin_1996,
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@article{Krumholz_2007,
  title = {Equations and {{Algorithms}} for {{Mixed-frame Flux-limited Diffusion Radiation Hydrodynamics}}},
  author = {{Krumholz}, Mark R. and {Klein}, Richard I. and {McKee}, Christopher F. and {Bolstad}, John},
  year = {2007},
  month = sep,
  journal = {The Astrophysical Journal},
  volume = {667},
  pages = {626--643},
  issn = {0004-637X},
  doi = {10.1086/520791},
  url = {https://ui.adsabs.harvard.edu/abs/2007ApJ...667..626K},
  urldate = {2023-10-18},
  abstract = {We analyze the mixed-frame equations of radiation hydrodynamics under the approximations of flux-limited diffusion and a thermal radiation field and derive the minimal set of evolution equations that includes all terms that are of leading order in any regime of nonrelativistic radiation hydrodynamics. Our equations are accurate to first order in v/c in the static diffusion regime. In contrast, we show that previous lower order derivations of these equations omit leading terms in at least some regimes. In comparison to comoving-frame formulations of radiation hydrodynamics, our equations have the advantage that they manifestly conserve total energy, making them very well suited to numerical simulations, particularly with adaptive meshes. For systems in the static diffusion regime, our analysis also suggests an algorithm that is both simpler and faster than earlier comoving-frame methods. We implement this algorithm in the Orion adaptive mesh refinement code and show that it performs well in a range of test problems.},
  keywords = {Astrophysics,Hydrodynamics,Methods: Numerical,Radiative Transfer},
  annotation = {ADS Bibcode: 2007ApJ...667..626K},
  file = {/Users/cche/Googledrive2/Academic/Zotero/Code/QUOKKA/Krumholz_plus_2007_Equations_and_Algorithms_for_Mixed-frame2.pdf}
}

@ARTICLE{Wibking_2022,
       author = {{Wibking}, Benjamin D. and {Krumholz}, Mark R.},
        title = "{QUOKKA: a code for two-moment AMR radiation hydrodynamics on GPUs}",
      journal = {\mnras},
     keywords = {hydrodynamics, methods: numerical, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2022,
        month = may,
       volume = {512},
       number = {1},
        pages = {1430-1449},
          doi = {10.1093/mnras/stac439},
archivePrefix = {arXiv},
       eprint = {2110.01792},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.1430W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{He_2024,
       author = {{He}, Chong-Chong and {Wibking}, Benjamin D. and {Krumholz}, Mark R.},
        title = "{An asymptotically correct implicit-explicit time integration scheme for finite volume radiation-hydrodynamics}",
      journal = {\mnras},
     keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2024,
        month = jun,
       volume = {531},
       number = {1},
        pages = {1228-1242},
          doi = {10.1093/mnras/stae1244},
archivePrefix = {arXiv},
       eprint = {2404.08247},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024MNRAS.531.1228H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{He_2024b,
       author = {{He}, Chong-Chong and {Wibking}, Benjamin D. and {Krumholz}, Mark R.},
        title = "{A novel numerical method for mixed-frame multigroup radiation-hydrodynamics with GPU acceleration implemented in the QUOKKA code}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Plasma Physics, Physics - Space Physics},
         year = 2024,
        month = jul,
          eid = {arXiv:2407.18304},
        pages = {arXiv:2407.18304},
archivePrefix = {arXiv},
       eprint = {2407.18304},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv240718304H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{He_2026,
       author = {{He}, Chong-Chong and {Wibking}, Benjamin D. and {Vijayan}, Aditi and {Krumholz}, Mark R. and {Li}, Pak Shing},
        title = "{A novel algorithm for GPU-accelerated particle-mesh interactions implemented in the QUOKKA code}",
      journal = {The Open Journal of Astrophysics},
     keywords = {Instrumentation and Methods for Astrophysics, Astrophysics of Galaxies},
         year = 2026,
        month = mar,
       volume = {9},
        pages = {159235},
          doi = {10.33232/001c.159235},
archivePrefix = {arXiv},
       eprint = {2509.18261},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2026OJAp....959235H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Vijayan_2024,
       author = {{Vijayan}, Aditi and {Krumholz}, Mark R. and {Wibking}, Benjamin D.},
        title = "{QUOKKA-based understanding of outflows (QED) - I. Metal loading, phase structure, and convergence testing for solar neighbourhood conditions}",
      journal = {\mnras},
     keywords = {methods: numerical, ISM: jets and outflows, galaxies: abundances, galaxies: evolution, galaxies: ISM, Astrophysics - Astrophysics of Galaxies},
         year = 2024,
        month = feb,
       volume = {527},
       number = {4},
        pages = {10095-10110},
          doi = {10.1093/mnras/stad3816},
archivePrefix = {arXiv},
       eprint = {2309.07955},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024MNRAS.52710095V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Huang_2025,
       author = {{Huang}, Rongjun and {Vijayan}, Aditi and {Krumholz}, Mark R.},
        title = "{QUOKKA-based understanding of outflows (QED) - II}",
      journal = {\mnras},
     keywords = {methods: data analysis, methods: numerical, X-rays: galaxies, Astrophysics of Galaxies},
         year = 2025,
        month = may,
       volume = {539},
       number = {2},
        pages = {1723-1737},
          doi = {10.1093/mnras/staf593},
archivePrefix = {arXiv},
       eprint = {2410.14376},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025MNRAS.539.1723H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Vijayan_2025,
       author = {{Vijayan}, Aditi and {Krumholz}, Mark R. and {Wibking}, Benjamin D.},
        title = "{QUOKKA-based understanding of outflows (QED) - III}",
      journal = {\mnras},
     keywords = {ISM: jets and outflows, ISM: structure, galaxies: ISM, galaxies: starburst, Astrophysics - Astrophysics of Galaxies},
         year = 2025,
        month = may,
       volume = {539},
       number = {2},
        pages = {1706-1722},
          doi = {10.1093/mnras/staf136},
archivePrefix = {arXiv},
       eprint = {2502.00929},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025MNRAS.539.1706V},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
