J/MNRAS/387/1099  Spectroscopic study of 10 high SB galaxies   (Pizzella+, 2008)

Structure and dynamics of galaxies with a low surface-brightness disc. I. The stellar and ionized-gas kinematics. Pizzella A., Corsini E.M., Sarzi M., Magorrian J., Mendez-Abreu J., Coccato L., Morelli L., Bertola F. <Mon. Not. R. Astron. Soc., 387, 1099-1116 (2008)> =2008MNRAS.387.1099P 2008MNRAS.387.1099P
ADC_Keywords: Galaxies, rotation ; Radial velocities Keywords: galaxies: kinematics and dynamics - galaxies: photometry - galaxies: spiral - galaxies: structure Abstract: Photometry and long-slit spectroscopy are presented for a sample of six galaxies with a low surface-brightness stellar disc and a bulge. The characterizing parameters of the bulge and disc components were derived by means of a two-dimensional photometric decomposition of the images of the sample galaxies. Their surface-brightness distribution was assumed to be the sum of the contribution of a Sersic bulge and an exponential disc, with each component being described by elliptical and concentric isophotes of constant ellipticity and position angle. The stellar and ionized-gas kinematics were measured along the major and minor axes in half of the sample galaxies, whereas the other half was observed only along two diagonal axes. Spectra along two diagonal axes were obtained also for one of the objects with major and minor axis spectra. The kinematic measurements extend in the disc region out to a surface-brightness level muR∼24mag/arcsec2, reaching in all cases the flat part of the rotation curve. The stellar kinematics turns out to be more regular and symmetric than the ionized-gas kinematics, which often shows the presence of non-circular, off-plane and non-ordered motions. This raises the question about the reliability of the use of the ionized gas as the tracer of the circular velocity in the modelling of the mass distribution, in particular in the central regions of low surface-brightness galaxies. Description: The photometric and spectroscopic data of the sample galaxies were obtained at the very large telescope (VLT) of the European Southern Observatory (ESO) at Paranal Observatory during three different runs between 2001 and 2003. The observations were carried out in service mode on May 05 - 2001 July 03 (run 1), April 13 - 2002 June 03 (run 2) and 2002 October 30 - 2003 February 04 (run 3). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file galaxies.dat 63 10 Studied galaxies table7.dat 65 182 Stellar kinematics of the sample galaxies table8.dat 50 730 Ionized-gas kinematics of the sample galaxies tablea6.dat 65 375 Stellar kinematics of the high SB galaxies tablea7.dat 50 717 Ionized-gas kinematics of the high SB galaxies -------------------------------------------------------------------------------- See also: VII/115 : Surface Photometry of ESO-Uppsala Galaxies (Lauberts+ 1989) J/A+A/342/671 : Early-type spiral galaxies kinematics (Corsini+ 1999) J/A+AS/120/257 : Ionized gas velocity in 6 galaxies (Zeilinger+ 1996) J/AJ/119/2540 : Asiago-ESO/RASS QSO survey. I. (Grazian+, 2000) J/A+A/360/439 : Stellar and ionized gas kinematics in NGC 4672 (Sarzi+, 2000) J/A+A/374/394 : Gas and stars kinematics in disc galaxies (Vega Beltran+ 2001) J/A+A/382/488 : Stellar and ionized gas kinematics in NGC 2855 (Corsini+ 2002) J/A+A/408/873 : Gas and stellar kinematics in spirals (Corsini+, 2003) J/A+A/416/507 : Minor-axis velocity gradients in disk galaxies (Coccato+ 2004) J/A+A/424/447 : Kinematics in 17 nearby spiral galaxies (Pizzella+, 2004) J/A+A/440/107 : Gas velocity curve along five spiral galaxies (Coccato+, 2005) J/A+A/482/53 : Radial velocities of four LSB galaxies (Pizzella+, 2008) J/A+A/497/41 : Average Early-type galaxies NIR spectrum (Cesetti+, 2009) Byte-by-byte Description of file: galaxies.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- ESO-LV ESO-LV designation 9- 10 I2 h RAh Simbad Hour of Right Ascension (J2000.0) 12- 13 I2 min RAm Simbad Minute of Right Ascension (J2000.0) 15- 18 F4.1 s RAs Simbad Second of Right Ascension (J2000.0) 20 A1 --- DE- Simbad Sign of the Declination (J2000.0) 21- 22 I2 deg DEd Simbad Degree of Declination (J2000.0) 24- 25 I2 arcmin DEm Simbad Arcminute of Declination (J2000.0) 27- 28 I2 arcsec DEs Simbad Arcsecond of Declination (J2000.0) 32- 36 F5.2 mag Bmag Simbad B band magnitude 38- 42 F5.2 mag Vmag ? Simbad V band magnitude 44- 46 A3 --- MType Simbad morphological type 48- 61 A14 --- SName Simbad name 63 A1 --- Sample [sh] s for sample galaxies (tables 7 and 8), h for high SB galaxies (tables a6 and a7) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat tablea6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- ESO-LV ESO-LV galaxy number 9- 11 I3 deg PA Position angle on the sky 13- 18 F6.2 arcsec r Distance from the galaxy center 20- 25 F6.1 km/s Vel Velocity 28- 31 F4.1 km/s e_Vel rms uncertainty on Vel 33- 37 F5.1 km/s sigma Velocity dispersion 40- 43 F4.1 km/s e_sigma rms uncertainty on sigma 45- 49 F5.2 --- h3 coefficient of 3rd-order Hermite polynomial 51- 54 F4.2 --- e_h3 rms uncertainty on h3 56- 60 F5.2 --- h4 coefficient if 4th-order Hermite polynomial 62- 65 F4.2 --- e_h4 rms uncertainty on h4 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat tablea7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- ESO-LV ESO-LV galaxy number 9- 11 I3 deg PA Position angle on the sky 13- 19 F7.2 arcsec r Distance from the galaxy center 21- 26 F6.1 km/s Vel Velocity 29- 32 F4.1 km/s e_Vel rms uncertainty on Vel 34- 38 F5.1 km/s sigma Velocity dispersion 41- 44 F4.1 km/s e_sigma Error on sigma (lower limit) 46- 50 F5.1 km/s E_sigma Error on sigma (upper limit) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 02-Jan-2010
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