- The SILCC (SImulating the LifeCycle of molecular Clouds) project II. …
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The SILCC (SImulating the LifeCycle of molecular Clouds) project II. Dynamical evolution of the supernova-driven ISM and the launching of outflows

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    SYSNO ASEP0472002
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThe SILCC (SImulating the LifeCycle of molecular Clouds) project II. Dynamical evolution of the supernova-driven ISM and the launching of outflows
    Author(s) Girichidis, P. (DE)
    Walch, S. (DE)
    Naab, T. (DE)
    Gatto, A. (DE)
    Wünsch, Richard (ASU-R) RID, ORCID
    Glover, S.C.O. (DE)
    Klessen, R.S. (DE)
    Clark, P.C. (DE)
    Peters, T. (DE)
    Derigs, D. (DE)
    Baczynski, C. (US)
    Source TitleMonthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711
    Roč. 456, č. 4 (2016), s. 3432-3455
    Number of pages24 s.
    Publication formPrint - P
    Languageeng - English
    CountryGB - United Kingdom
    Keywordshydrodynamics ; magnetic fields ; numerical methods
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGAP209/12/1795 GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000372265800004
    EID SCOPUS84963807262
    DOI https://doi.org/10.1093/mnras/stv2742
    AnnotationThe SILCC project (SImulating the Life-Cycle of molecular Clouds) aims at a more self-consistent understanding of the interstellar medium (ISM) on small scales and its link to galaxy evolution. We present three-dimensional (magneto) hydrodynamic simulations of the ISM in a vertically stratified box including self-gravity, an external potential due to the stellar component of the galactic disc, and stellar feedback in the form of an interstellar radiation field and supernovae (SNe). The cooling of the gas is based on a chemical network that follows the abundances of H+, H, H-2, C+, and CO and takes shielding into account consistently. We vary the SN feedback by comparing different SN rates, clustering and different positioning, in particular SNe in density peaks and at random positions, which has a major impact on the dynamics.
    WorkplaceAstronomical Institute
    ContactAnežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2017
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