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Galactic winds driven by cosmic ray streaming
Galactic winds are observed in many spiral galaxies with sizes from dwarfs up to the Milky Way, and they sometimes carry a mass in excess of that of newly formed stars by up to a factor of ten. Multiple driving processes of such winds have been proposed,
Christoph Pfrommer, Torsten A Enßlin
exaly +3 more sources
CLASSY. VI. The Density, Structure, and Size of Absorption-line Outflows in Starburst Galaxies
Galaxy formation and evolution are regulated by the feedback from galactic winds. Absorption lines provide the most widely available probe of winds.
Xinfeng Xu +14 more
doaj +1 more source
Resolved Velocity Profiles of Galactic Winds at Cosmic Noon
We study the kinematics of the interstellar medium (ISM) viewed “down the barrel” in 20 gravitationally lensed galaxies during cosmic noon ( z = 1.5–3.5).
Keerthi Vasan G. C. +9 more
doaj +1 more source
Galactic dynamos and galactic winds [PDF]
8 pages, 7 figures. To be published in "The UV Window to the Universe", eds. A.I. Gomez de Castro and M. Castellanos, Ap&SS Special Issue, Springer, Berlin.
openaire +2 more sources
Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds [PDF]
We investigate the efficiency and time-dependence of thermally and cosmic ray driven galactic winds for the metal enrichment of the intra-cluster medium (ICM) using a new analytical approximation for the mass outflow.
Abadi +72 more
core +2 more sources
Metal enrichment of the intra-cluster medium over a Hubble time for merging and relaxed galaxy clusters [PDF]
We investigate the efficiency of galactic mass loss, triggered by ram-pressure stripping and galactic winds of cluster galaxies, on the chemical enrichment of the intra-cluster medium (ICM).
Arnaud +66 more
core +2 more sources
Galactic Winds in Low-Mass Galaxies [PDF]
AbstractMass-loss via stellar-feedback driven outflows is predicted to play a critical role in the baryon cycle of low-mass galaxies. However, observational constraints on warm winds are limited as outflows are transient, intrinsically low-surface brightness events and, thus, difficult to detect.
Kristen. B. W. McQuinn +2 more
openaire +2 more sources
Magnetic Fields Around Galactic Discs
Magnetic fields in the discs of spiral galaxies are quite well understood, although, of course, many details still require investigation and future observations with new generations of radio telescopes will be valuable here.
David Moss, Dmitry Sokoloff
doaj +1 more source
We report on the discovery of a rare case of spatially and kinematically resolved galactic-scale outflow at intermediate redshift based on VLT/MUSE optical integral field spectroscopic observation of the quasar HE 0238–1904.
Qinyuan Zhao, Junfeng Wang
doaj +1 more source

