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- W4234929197 abstract "In the sequel we will be discussing that - apart from all other halo flows - it is highly probable that our Galaxy has a systematic mass loss; most other galaxies should behave in a similar way. This mass loss should occur in the form of a supersonic galactic wind provided the intergalactic pressure is low enough. We will investigate this possibility mainly for our Galaxy. We shall argue [1] that the energetic particle component of the interstellar medium, the cosmic rays (CRs), is basically responsible for driving a wind for typical gas temperatures below 10 6 K. Thus for asymptotic wind velocities of the order of the escape velocity, the mass flux is essentially determined by the observable CR energy loss from the Galaxy. Galaxies with very hot gas on the other hand hardly need the CR component and drive a wind almost exclusively through their thermal pressure." @default.
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- W4234929197 date "1989-01-01" @default.
- W4234929197 modified "2023-10-14" @default.
- W4234929197 title "Galactic Winds" @default.
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- W4234929197 doi "https://doi.org/10.1017/s0252921100024222" @default.
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