ISM simulations: an overview of models

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dc.contributor.authorde Avillez, Miguel
dc.contributor.authorBreitschwerdt, Dieter
dc.contributor.authorAsgekar, Ashish
dc.contributor.authorSpitoni, Emanuele
dc.date.accessioned2017-02-02T11:21:29Z
dc.date.available2017-02-02T11:21:29Z
dc.date.issued2015-03-16
dc.description.abstractUntil recently the dynamical evolution of the interstellar medium (ISM) was simu- lated using collisional ionization equilibrium (CIE) conditions. However, the ISM is a dynamical system, in which the plasma is naturally driven out of equilibrium due to atomic and dynamic processes operating on different timescales. A step forward in the field comprises a multi-fluid approach taking into account the joint thermal and dynamical evolutions of the ISM gas.por
dc.identifier.authoremailmavillez@uevora.pt
dc.identifier.authoremailnd
dc.identifier.authoremailnd
dc.identifier.authoremailnd
dc.identifier.doi10.1017/S1743921314012393por
dc.identifier.urihttps://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/div-classtitleism-simulations-an-overview-of-modelsdiv/3832BECA0284489C4AE6E079CA34EC6A
dc.identifier.urihttp://hdl.handle.net/10174/20577
dc.language.isoengpor
dc.peerreviewedyespor
dc.publisherHighlights of Astronomy/Cambridge university Presspor
dc.rightsopenAccesspor
dc.subjectISM: generalpor
dc.subjectISM: structurepor
dc.subjectatomic processespor
dc.subjectturbulencepor
dc.subjectMHDpor
dc.titleISM simulations: an overview of modelspor
dc.typearticlepor

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