========================================================================== J/MNRAS/362/301 Spectrophotometry of the HII region S311 (Garcia-Rojas+, 2005) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table2.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/362/301 ==========================================================================
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Beginning of ReadMe : J/MNRAS/362/301 Spectrophotometry of the HII region S311 (Garcia-Rojas+, 2005) ================================================================================ Deep echelle spectrophotometry of S311, a Galactic HII region located outside the solar circle. Garcia-Rojas J., Esteban C., Peimbert A., Peimbert M., Rodriguez M., Ruiz M.T. <Mon. Not. R. Astron. Soc., 362, 301-312 (2005)> =2005MNRAS.362..301G ================================================================================ ADC_Keywords: H II regions ; Spectrophotometry Keywords: ISM: abundances - H II regions - ISM: individual: S 311 Abstract: We present echelle spectrophotometry of the Galactic H II region S311. The data have been taken with the Very Large Telescope Ultraviolet-Visual Echelle Spectrograph in the 3100-10400AA range. We have measured the intensities of 263 emission lines; 178 are permitted lines of H^0^, D^0^ (deuterium), He^0^, C^0^, C^+^, N^0^, N^+^, O^0^, O^+^, S^+^, Si^0^, Si^+^, Ar^0^ and Fe^0^; some of them are produced by recombination and others mainly by fluorescence. Description: The observations were made on 2003 March 30 with the UVES, at the VLT Kueyen Telescope in Cerro Paranal Observatory (Chile). We used the standard settings in both the red and blue arms of the spectrograph, covering the region from 3100 to 10400AA. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 07 52 19.3 -26 26 30 Sh 2-311 = NGC 2467 ----------------------------------------------------------
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