Modelling the supernova-driven ISM in different environments

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00445330" target="_blank" >RIV/67985815:_____/15:00445330 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1093/mnras/stv324" target="_blank" >http://dx.doi.org/10.1093/mnras/stv324</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stv324" target="_blank" >10.1093/mnras/stv324</a>

Result language
angličtina
Original language name
Modelling the supernova-driven ISM in different environments
Original language description
We use hydrodynamical simulations in a (256 pc)(3) periodic box to model the impact of supernova (SN) explosions on the multiphase interstellar medium (ISM) for initial densities n = 0.5-30 cm(-3) and SN rates 1-720 Myr(-1). We include radiative cooling,diffuse heating, and the formation of molecular gas using a chemical network. The SNe explode either at random positions, at density peaks, or both. We further present a model combining thermal energy for resolved and momentum input for unresolved SNe.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/GAP209%2F12%2F1795" target="_blank" >GAP209/12/1795: Star formation triggered by expanding shells</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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