The Relation Between Optical Extinction and Hydrogen Column Density in the Galaxy

TL;DR

This study refines the linear relationship between hydrogen column density and optical extinction in the Galaxy using data from 22 supernova remnants observed with advanced X-ray observatories, providing a more precise slope estimate.

Contribution

It offers a new, more accurate measurement of the N_H-A_V relation based on recent high-quality data, addressing previous discrepancies.

Findings

Derived N_H (cm^-2) = (2.21 ± 0.09) x 10^{21} A_V (mag)

Compared results with previous studies to evaluate systematic uncertainties

Assessed the impact of observational uncertainties on the relation

Abstract

A linear relation between the hydrogen column density (N_H) and optical extinction (A_V) in the Galaxy has long been observed. A number of studies found differing results in the slope of this relation. Here, we utilize the data on 22 supernova remnants that have been observed with the latest generation X-ray observatories and for which optical extinction and/or reddening measurements have been performed and find N_H (cm^-2) = (2.21 \pm0.09) x10^{21} A_V (mag). We compare our result with the previous studies and assess any systematic uncertainties that may affect these results.