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- W4200634957 abstract "The effects of cosmic ray diffusion and radiative cooling on the structure of the Galactic wind are studied in steady state approximation. It is known that realistic cooling processes suppress the wind from launching. The effects of cosmic ray diffusion is also supposed to be unfavorable for launching the wind. Both of these effects have not been studied simultaneously in a steady state approximation of the wind. We find 327254 solutions of the steady state Galactic wind, and confirm that the effect of cosmic ray pressure depends on the Alfv'en Mach number, mass flux carried by the wind does not depend on the cosmic ray pressure directly (but depend on the thermal pressure), and typical condition found in the Galaxy may correspond to the wind solution that provide a metal polluted matters at a height of $sim300$ kpc from the disk." @default.
- W4200634957 created "2021-12-31" @default.
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- W4200634957 date "2021-12-09" @default.
- W4200634957 modified "2023-09-27" @default.
- W4200634957 title "The Effects of Cosmic Ray Diffusion and Radiative Cooling on the Galactic Wind from the Milky Way" @default.
- W4200634957 hasPublicationYear "2021" @default.
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