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dc.contributor.authorVandenbroucke, B.
dc.contributor.authorWood, K.
dc.date.accessioned2019-03-08T00:37:57Z
dc.date.available2019-03-08T00:37:57Z
dc.date.issued2018-04
dc.identifier.citationVandenbroucke , B & Wood , K 2018 , ' The Monte Carlo photoionization and moving-mesh radiation hydrodynamics code CMacIonize ' , Astronomy and Computing , vol. 23 , pp. 40-59 . https://doi.org/10.1016/j.ascom.2018.02.005en
dc.identifier.issn2213-1337
dc.identifier.otherPURE: 252065733
dc.identifier.otherPURE UUID: 04325dda-e3f6-4ae7-8806-7f93d41ec2d6
dc.identifier.otherScopus: 85045896539
dc.identifier.otherORCID: /0000-0001-7241-1704/work/50167446
dc.identifier.otherWOS: 000437094400004
dc.identifier.urihttp://hdl.handle.net/10023/17240
dc.descriptionWe acknowledge support from STFC grant ST/M001296/1.en
dc.description.abstractWe present the public Monte Carlo photoionization and moving-mesh radiation hydrodynamics code CMacIonize, which can be used to simulate the self-consistent evolution of HII regions surrounding young O and B stars, or other sources of ionizing radiation. The code combines a Monte Carlo photoionization algorithm that uses a complex mix of hydrogen, helium and several coolants in order to self-consistently solve for the ionization and temperature balance at any given type, with a standard first order hydrodynamics scheme. The code can be run as a post-processing tool to get the line emission from an existing simulation snapshot, but can also be used to run full radiation hydrodynamical simulations. Both the radiation transfer and the hydrodynamics are implemented in a general way that is independent of the grid structure that is used to discretize the system, allowing it to be run both as a standard fixed grid code, but also as a moving-mesh code.
dc.format.extent20
dc.language.isoeng
dc.relation.ispartofAstronomy and Computingen
dc.rights© 2018 Elsevier Ltd. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1016/j.ascom.2018.02.005en
dc.subjectNumericalen
dc.subjectHydrodynamicsen
dc.subjectRadiative transferen
dc.subjectISM: evolutionen
dc.subjectQA75 Electronic computers. Computer scienceen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subjectBDCen
dc.subject.lccQA75en
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe Monte Carlo photoionization and moving-mesh radiation hydrodynamics code CMacIonizeen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1016/j.ascom.2018.02.005
dc.description.statusPeer revieweden
dc.date.embargoedUntil2019-03-08


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