J/A+AS/139/483    Early-type gal. kinematics in compact groups (Bonfanti+, 1999)

Kinematics of early-type galaxies in compact groups. HCG 67, HCG 74, and HCG 79 Bonfanti, P., Simien, F., Rampazzo, R., Prugniel, P. <Astron. Astrophys. Suppl. Ser. 139, 483 (1999)> =1999A&AS..139..483B 1999A&AS..139..483B (SIMBAD/NED BibCode)
ADC_Keywords: Radial velocities ; Galaxies, rotation ; Velocity dispersion ; Clusters, galaxy Keywords: galaxies: kinematics & dynamics - galaxies: interactions - galaxies: elliptical and lenticular, cD - galaxies: formation - galaxies: evolution Abstract: We present measurements of stellar kinematics for seven early-type galaxies in HCG 67, HCG 74, and HCG 79. These data are aimed at studying the relation between the environment and the dynamics, structure and stellar content of early-type galaxies. In the present three groups, the kinematic features we observed cannot be associated unambiguously to physical interactions. Visible morphological peculiarities do not appear correlated with kinematical perturbations. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 13 49 11.3 -07 13 27.6 HCG 67a 13 49 09.7 -07 13 54.3 HCG 67d 15 19 24.7 +21 06 20.3 HCG 74a 15 19 24.4 +20 53 23.4 HCG 74b 15 59 11.4 +20 45 14.9 HCG 79a 15 59 12.6 +20 45 47.1 HCG 79b 15 59 10.9 +20 45 41.4 HCG 79c ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 24 7 Main kinematical parameters from this study table4.dat 38 182 Profiles of rotation and velocity dispersion -------------------------------------------------------------------------------- See also: J/A+AS/122/521 : Kinematical data on early-type galaxies. I. (Simien+ 1997) J/A+AS/126/15 : Kinematical data on early-type galaxies. II. (Simien+ 1997) J/A+AS/126/519 : Kinematical data on early-type galaxies. III. (Simien+ 1997) J/A+AS/131/287 : Kinematical data on early-type galaxies. IV. (Simien+ 1998) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object identification 10- 14 I5 km/s V0hel Heliocentric systemic velocity 16- 17 I2 km/s e_V0hel Mean error on V0hel (rms) 19- 21 I3 km/s sigma0 Projected central velocity dispersion 23- 24 I2 km/s e_sigma0 Mean error on sigma0 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object identification 11- 13 I3 deg PA Position angle of slit (1) 15- 20 F6.1 arcsec r Radius (<0 and >0 on opposite semi-axes) (1) 22- 26 I5 km/s Vrot ?=999 Proj. mean stellar rotation velocity (2) 28- 30 I3 km/s e_Vrot ?=999 Mean error on Vrot 32- 34 I3 km/s sigma ?=999 Projected velocity dispersion (2) 36- 38 I3 km/s e_sigma ?=999 Mean error on sigma -------------------------------------------------------------------------------- Note (1): Rotation and dispersion velocities are projected along the line of sight; rotation values are with respect to the point r=0 of the component whose identification is given in bytes 1-9. Note (2): For HCG67a, HCG79a, and HCG79b, PA has been shifted +180 degrees with respect to the printed version, in order to conform to the convention used by Simien & Prugniel (1997, Cat. J/A+AS/126/519), which is recalled below. PA (North --> East) is in the range [0, 360[, and: - for 0<PA<180, r<0 corresponds to the eastern side of the galaxy, - for 180<PA<360, r<0 corresponds to the western side, - and for PA=0, r<0 is to the North. -------------------------------------------------------------------------------- Acknowledgements: Francois Simien
(End) Patricia Bauer [CDS] 19-Oct-1999
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