J/A+AS/124/61              Stellar Rotation in SB0 galaxies      (Bettoni+ 1997)

A survey of the stellar rotation in barred galaxies Bettoni D., Galletta G. <Astron. Astrophys. Suppl. Ser. 124, 61 (1997)> =1997A&AS..124...61B 1997A&AS..124...61B
ADC_Keywords: Radial velocities ; Velocity dispersion Keywords: galaxies: kinematics and dynamics - galaxies: elliptical and lenticular Abstract: We present stellar velocity- and velocity dispersion- data for 13 SB0 galaxies and one SBa, based on 61 spectra collected during a long-term project developed at ESO. Our primary goal is to provide a database widest as possible for the study of the stellar velocity and velocity dispersion fields and for future modeling. New data are presented for six galaxies, while for the remaining SB0s particular kinematical aspects were already discussed in previous papers. We found the following results: a) emission lines were detected in our spectra only for 4 out of 14 galaxies considered. When present, they reveal a very peculiar kinematics, including counter-rotation, warps or radial flows. b) A new case of gas counter-rotation has been found: NGC 7079. c) The velocity dispersion along the bar has a smoother trend than in the rest of the galaxy. However there is, in general, a similarity between the velocity dispersion trend (decreasing or flat) measured along the bar and that outside it. d) The existence of a waving pattern in the stellar rotation curves of bars is confirmed for the galaxies of our sample seen inclined between 30 and 50°. In addition to this effect, the percentage of non-circular stellar motions present in the barred galaxies studied may reach the 20%. Description: We present stellar velocity- and velocity dispersion- data for 13 SB0 galaxies and one SBa, based on 61 spectra collected at ESO. We want to provide a database for the study of the stellar velocity and velocity dispersion fields and for future modeling. In the Table radii are in arcsec, velocity and velocity dispersion are in Km/s File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file galaxies.dat 32 14 List of studied galaxies table5.dat 44 2449 Kinematical data for the sample galaxies table5.tex 75 2965 LaTeX version of table5 -------------------------------------------------------------------------------- Byte-by-byte Description of file: galaxies.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Galaxy name 10- 11 I2 h RAh Hour of Right Ascension (J2000) 13- 14 I2 min RAm Minute of Right Ascension (J2000) 16- 20 F5.2 s RAs Second of Right Ascension (J2000) 22 A1 --- DE- Sign of the Declination (J2000) 23- 24 I2 deg DEd Degree of Declination (J2000) 26- 27 I2 arcmin DEm Arcminute of Declination (J2000) 29- 32 F4.1 arcsec DEs Arcsecond of Declination (J2000) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Galaxy name 10- 12 I3 deg PA Position angle of the spectrograph slit 14- 17 A4 --- Oslit Offset of the slit with respect to the nucleus (4"NW, 4"SE, 5"NW, or 5"SE) 18- 19 I2 min Exp ? Exposure time 21- 26 F6.1 arcsec Rad [-108.5/110.3] Radius 28- 31 I4 km/s HRV Heliocentric radial velocity 33- 35 I3 km/s e_HRV rms uncertainty on HRV 37- 40 I4 km/s sigma Velocity dispersion σ 42- 44 I3 km/s e_sigma rms uncertainty on sigma -------------------------------------------------------------------------------- Acknowledgements: Daniela Bettoni
(End) Patricia Bauer [CDS] 31-Oct-1996
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line