J/A+A/416/475       Long slit spectroscopy of HII regions    (Marquez+, 2004)

Long slit spectroscopy of a sample of isolated spirals with and without an AGN. Marquez I., Durret F., Masegosa J., Moles M., Varela J., Gonzalez Delgado R.M., Maza J., Perez E., Roth M. <Astron. Astrophys. 416, 475 (2004)> =2004A&A...416..475M 2004A&A...416..475M
ADC_Keywords: H II regions ; Equivalent widths ; Spectroscopy Keywords: galaxies: spiral - galaxies: kinematics and dynamics - galaxies: structure - galaxies: interaction Abstract: We present the kinematical data obtained for a sample of active (Seyfert) and non active isolated spiral galaxies, based on long slit spectra along several position angles in the Hα line region and, in some cases, in the Ca triplet region as well. Gas velocity distributions are presented, together with a simple circular rotation model that allows us to determine the kinematical major axes. Stellar velocity distributions are also shown. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 80 224 Emission line measurements for the 224 HII regions for 20 galaxies of our sample having Hα equivalent widths larger than 10Å -------------------------------------------------------------------------------- See also: J/ApJS/112/29 : HII regions in southern spiral galaxies (Feinstein 1997) J/A+A/393/389 : Hα in HII regions in spiral galaxies (Marquez+, 2002) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Galaxy Galaxy name 12- 14 I3 deg PA Slit position angle, anti-clockwise from north 16- 21 F6.1 arcsec Dist Distance to the nucleus along the slit (1) 23- 29 F7.3 0.1nm EWHa Hα equivalent width 31- 35 F5.3 --- [OI]/Ha ? [OI]λ6300/Hα line intensity ratio 37- 41 F5.3 --- e_[OI]/Ha ? rms uncertainty on [OI]/Ha 43- 47 F5.3 --- [NII]/Ha Intensity ratio [NII]λ6584/Hα 49- 53 F5.3 --- e_[NII]/Ha rms uncertainty on [NII]/Ha 55- 61 F7.3 --- [SII]/Ha Intensity ratio [SII]λ6717+6731/Hα 63- 67 F5.3 --- e_[SII]/Ha rms uncertainty on [SII]/Ha 69- 76 F8.3 --- [SII]/[SII] Intensity ratio [SII]λ6717/[SII]λ6731 -------------------------------------------------------------------------------- Note (1): Negative (positive) values correspond to the regions left (right) of the nucleus on the velocity curves drawn for the corresponding slits. -------------------------------------------------------------------------------- Acknowledgements: Florence Durret
(End) Patricia Bauer [CDS] 19-Dec-2003
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