SILCC - VII. Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00573379" target="_blank" >RIV/67985815:_____/23:00573379 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stad1104" target="_blank" >https://doi.org/10.1093/mnras/stad1104</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stad1104" target="_blank" >10.1093/mnras/stad1104</a>

Result language
angličtina
Original language name
SILCC - VII. Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
Original language description
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase interstellar medium (ISM) in stratified galactic patches with gas surface densities ∑gas = 10, 30, 50, and 100 M☉ pc−2. The SILCC project simulation framework accounts for non-equilibrium thermal and chemical processes in the warm and cold ISM. The sink-based star formation and feedback model includes stellar winds, hydrogen-ionizing UV radiation, core-collapse supernovae, and cosmic ray (CR) injection and diffusion. The simulations follow the observed relation between ∑gas and the star formation rate surface density ∑SFR. CRs qualitatively change the outflow phase structure.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA20-19854S" target="_blank" >GA20-19854S: Particle Acceleration Studies in Astrophysical Jets</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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