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- W2894774942 abstract "The role of magnetic fields in the multi-phase interstellar medium (ISM) is explored using magnetohydrodynamic (MHD) simulations that include energy injection by supernova (SN) explosions and allow for dynamo action. Apart from providing additional pressure support of the gas layer, magnetic fields reduce the density contrast between the warm and hot gas phases and quench galactic outflows. A dynamo-generated, self-consistent large-scale magnetic field affects the ISM differently from an artificially imposed, unidirectional magnetic field." @default.
- W2894774942 created "2018-10-12" @default.
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- W2894774942 date "2018-10-02" @default.
- W2894774942 modified "2023-09-25" @default.
- W2894774942 title "Magnetic field effects on the ISM structure and galactic outflows" @default.
- W2894774942 doi "https://doi.org/10.48550/arxiv.1810.01202" @default.
- W2894774942 hasPublicationYear "2018" @default.
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