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Oxygen and helium abundances in Galactic H ii regions – I. Observations
Authors:J Caplan  L Deharveng  M Peña  R Costero  C Blondel
Institution:Observatoire de Marseille, 2 place Le Verrier, 13248 Marseille Cedex 4, France; Instituto de Astronomía, UNAM, Apdo. Postal 70-264, Cd. Universitaria, 04510 México, D.F., México; Service d'Astrophysique, DAPNIA, CEA/Saclay, 91191 Gif-sur-Yvette Cedex, France
Abstract:Absolute integrated line fluxes of H  ii regions have been measured using a Fabry–Perot spectrophotometer. We describe the observations and calibration procedures. Fluxes are given for 36 H  ii regions with Galactocentric distances ranging from 6.6 to 17.7 kpc. Several emission lines have been measured, mainly O  ii ] λλ 3726 and 3629, H β , O  iii ] λ 5007, He  i λ 5876 and H α . The very faint O  iii ] λ 4363 line has been measured in six regions, allowing a direct determination of the electron temperature. New photometric distances have been derived based on data from the literature. A discussion of these results in terms of extinction, electron density and temperature, and oxygen and helium abundances is given in Paper II.
Keywords:instrumentation: miscellaneous  techniques: photometric  ISM: abundances  H ii regions
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