Visual extinction towards the Omega Nebula (M17) and the ionization of nitrogen in the nebula

We estimate the absolute intensity of the Hα emission line in M17 based on spectroscopic observations with the 70 cm telescope of the Fesenkov Astrophysical Institute and the 1.25 m telescope of the Sternberg Astronomical Institute’s Crimean Laboratory. The visual extinction, A _v , is derived for about 250 regions in the nebula via a comparison of the optical (Hα) and radio (21 cm continuum) emissions. The A _v values for the eastern, optically bright, part of the nebula are 2–6^m. For the western part, which is covered by a dark cloud, the extinction is A _v = 7?14.5^m. We derived I(Hα)/I([NII] λ6584) ratios and estimated the degree of ionization of nitrogen in the nebula; we find that most nitrogen is in the [NIII] state.