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Paper detail

The low density and magnetization of a massive galaxy halo exposed by a fast radio burst

Present-day galaxies are surrounded by cool and enriched halo gas extending to hundreds of kiloparsecs. This halo gas is thought to be the dominant reservoir of material available to fuel future star formation, but direct constraints on its mass and physical properties have been difficult to obtain. We report the detection of a fast radio burst (FRB 181112) with arcsecond precision, which passes through the halo of a foreground galaxy. Analysis of the burst shows the halo gas has low net magnetization and turbulence. Our results imply predominantly diffuse gas in massive galactic halos, even those hosting active supermassive black holes, contrary to some previous results.

preprint2019arXivOpen access
J. Xavier ProchaskaJean-Pierre MacquartMatthew McQuinnSunil SimhaRyan M. ShannonCherie K. DayLachlan MarnochStuart RyderAdam DellerKeith W. BannisterShivani BhandariRongmon BordoloiJohn BuntonHyerin ChoChris FlynnElizabeth K. MahonyChris PhillipsHao QiuNicolas Tejos
astro-ph.GA
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J. Xavier ProchaskaJean-Pierre MacquartMatthew McQuinnSunil SimhaRyan M. ShannonCherie K. DayLachlan MarnochStuart RyderAdam DellerKeith W. BannisterShivani BhandariRongmon BordoloiJohn BuntonHyerin ChoChris FlynnElizabeth K. MahonyChris PhillipsHao QiuNicolas Tejos

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