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• W2116996854 abstract "We present new echelle spectrophotometry of the Galactic H II regions M8 and M17. The data have been taken with the VLT UVES echelle spectrograph in the 3100 to 10400 A range. We have measured the intensities of 375 and 260 emission lines in M8 and M17 respectively, increasing signicativ ely the number of emission lines measured in previous spectrophotometric studies of these nebulae. Most of the detected lines are permitted lines. Electron temperatures and densities have been determined using dieren t diagnostics. We have derived He + , C ++ , O + and O ++ ionic abundances from pure recombination lines. We have also derived abundances from collisionally excited lines for a large number of ions of dieren t elements. Highly consistent estimations of t 2 have been obtained by using dieren t independent indicators; the values are moderate and very similar to those obtained in other Galactic H II regions. We report the detection of deuterium Balmer emission lines, up to D , in M8 and show that their intensities are consistent with continuum uorescence as their main excitation mechanism." @default.
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• W2116996854 date "2007-01-01" @default.
• W2116996854 modified "2023-10-02" @default.
• W2116996854 title "The Chemical Composition of the Galactic H II Regions M8 and M17. A Revision based on deep VLT Echelle Spectrophotometry" @default.
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