An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB

The CHIME/FRB project has detected hundreds of fast radio bursts (FRBs), providing an unparalleled population to statistically probe the foreground media that they illuminate. One such foreground medium is the ionized halo of the Milky Way (MW). We estimate the total Galactic electron column density from FRB dispersion measures (DMs) as a function of Galactic latitude using four different estimators, including ones that assume spherical symmetry of the ionized MW halo and ones that imply more latitudinal variation in density. Our observation-based constraints of the total Galactic DM contribution for divide b divide >= 30 degrees, depending on the Galactic latitude and selected model, span 87.8-141 pc cm(-3). This constraint implies upper limits on the MW halo DM contribution that range over 52-111 pc cm(-3). We discuss the viability of various gas density profiles for the MW halo that have been used to estimate the halo's contribution to DMs of extragalactic sources. Several models overestimate the DM contribution, especially when assuming higher halo gas masses (similar to 3.5 x 10(12) M (circle dot)). Some halo models predict a higher MW halo DM contribution than can be supported by our observations unless the effect of feedback is increased within them, highlighting the impact of feedback processes in galaxy formation.

Automated summary

The CHIME/FRB project has used the detected fast radio bursts to study the foreground media, such as the ionized halo of the Milky Way. They estimated the total electron column density of the Galactic halo from the dispersion measures of FRBs at different Galactic latitudes. The constraints from their observations imply upper limits on the contribution of the Milky Way halo, highlighting the impact of feedback processes in galaxy formation.