SIMBAD references

We investigate the relation between the optical extinction (A_V) and the hydrogen column density (N_H) determined from X-ray observations of a large sample of Galactic sightlines towards 35 supernova remnants, 6 planetary nebulae and 70 X-ray binaries for which N_H was determined in the literature with solar abundances. We derive an average ratio of <N_H/A_V> = (2.08 ± 0.02) x 10²¹ H cm^–2 mag^–1 for the whole Galaxy. We find no correlation between <N_H/A_V> and the number density of hydrogen, the distance away from the Galactic Centre and the distance above or below the Galactic plane. The <N_H/A_V> ratio is generally invariant across the Galaxy, with <N_H/A_V> = (2.04 ± 0.05) x 10²¹ H cm^–2 mag^–1 for the first and fourth Galactic quadrants and <N_H/A_V> = (2.09 ± 0.03) x 10²¹ H cm^–2 mag^–1 for the second and third Galactic quadrants. We also explore the distribution of hydrogen in the Galaxy by enlarging our sample with additional 74 supernova remnants for which both N_H and distances are known. We find that, between the Galactic radius of 2 and 10 kpc, the vertical distribution of hydrogen can be roughly described by a Gaussian function with a scaleheight of h = 75.5 ± 12.4 pc and a mid-plane density of n_H(0) = 1.11 ± 0.15 cm^–3, corresponding to a total gas surface density of ∑_gas ∼ 7.0 M_☉ pc^–2. We also compile N_H from 19 supernova remnants and 29 X-ray binaries for which N_H was determined with subsolar abundances. We obtain <N_H/A_V> = (2.47 ± 0.04) x 10²¹ H cm^–2 mag^–1 which exceeds that derived with solar abundances by ∼20 per cent. We suggest that in future studies one may simply scale N_H derived from subsolar abundances by a factor of ∼1.2 when converting to N_H of solar abundances.