A single HII region model of the strong interstellar scattering towards Sgr A*

TL;DR

This paper proposes that a single HII region located 1.5-4.8 kpc from Earth explains the strong interstellar scattering observed towards Sgr A*, challenging previous assumptions that the scattering originated near the Galactic center.

Contribution

The study introduces a model where a single HII region accounts for the scattering, providing constraints on its location, properties, and effects on observed pulsar signals and spectra.

Findings

HII region at 1.5-4.8 kpc explains scattering of Sgr A*

Model predicts similar scattering for sources within 10 pc

HII region can produce observed rotation measure without strong magnetisation

Abstract

Until recently, the strong interstellar scattering observed towards the Galactic center (GC) black hole, Sgr A*, was thought to come from dense gas within the GC region. The pulse broadening towards the transient magnetar SGR J1745-2900 near Sgr A* has shown that the source of the scattering is instead located much closer to Earth, possibly in a nearby spiral arm. We show that a single HII region along the line of sight, 1.5-4.8 kpc away from Earth with density $n_e$ of a few 100 cm$^{-3}$ and radius R = 1.8-3.2 pc can explain the observed angular broadening of Sgr A*. Clouds closer to the GC overproduce the observed DM, providing an independent location constraint that agrees with that from the magnetar pulse broadening. Our model predicts that sources within 10 pc should show the same scattering origin as the magnetar and Sgr A*, while the nearest known pulsars with separations > 20 pc should not. The radio spectrum of Sgr A* should show a cutoff from free-free absorption at 0.2-1 GHz. For a magnetic field strength $B = 15-70 \mu$G, the HII region could produce the rotation measure of the magnetar, the largest of any known pulsar, without requiring the gas near Sgr A* to be strongly magnetised.