J/MNRAS/391/1009  Radial kinematics in bright cluster galaxies (Loubser+ 2008)

Radial kinematics of brightest cluster galaxies. Loubser S.I., Sansom A.E., Sanchez-Blazquez P., Soechting I.K., Bromage G.E. <Mon. Not. R. Astron. Soc., 391, 1009-1028 (2008)> =2008MNRAS.391.1009L 2008MNRAS.391.1009L
ADC_Keywords: Clusters, galaxy ; Radial velocities ; Velocity dispersion Keywords: galaxies: elliptical and lenticular, cD - galaxies: kinematics and dynamics Abstract: This is the first of a series of papers devoted to the investigation of a large sample of brightest cluster galaxies (BCGs), their kinematic and stellar population properties, and the relationships between those and the properties of the cluster. We have obtained high signal-to-noise ratio, long-slit spectra of these galaxies with Gemini and William Herschel Telescope with the primary purpose of investigating their stellar population properties. This paper describes the selection methods and criteria used to compile a new sample of galaxies, concentrating on BCGs previously classified as containing a halo (cD galaxies), together with the observations and data reduction. Here, we present the full sample of galaxies, and the measurement and interpretation of the radial velocity and velocity dispersion profiles of 41 BCGs. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 116 65 The new sample of BCGs rv/* . 43 Individual radial kinematics files -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Name Galaxy name 14 A1 --- n_Name [*] * for ordinary ellipticals 16- 17 I2 h RAh Right ascension (J2000) 19- 20 I2 min RAm Right ascension (J2000) 22- 25 F4.1 s RAs RAs Right ascension (J2000) 27 A1 --- DE- Declination sign (J2000) 28- 29 I2 deg DEd Declination (J2000) 31- 32 I2 arcmin DEm Declination (J2000) 34- 35 I2 arcsec DEs Declination (J2000) 36- 51 A16 --- Cluster Cluster name 53- 70 A18 --- MType NED morphological type (1) 72- 75 F4.1 --- TType ?=- T morphological type 77- 79 F3.1 --- e_TType ? rms uncertainty on TType 81- 83 I3 deg PA ?=- Position angle of the galaxy major axis 85- 89 F5.2 mag Bmag B magnitude 91- 96 F6.2 mag BMAG ?=- Absolute B magnitude 98-101 A4 --- Ref Reference for search method (2) 103 I1 --- Run ? Run number 105-116 A12 --- FileName Name of the file with radial kinematic data in subdirectory rv -------------------------------------------------------------------------------- Note (1): Besides the galaxies classified as cD/D in the NED morphology, NGC 6034, UGC 05515 and NGC 1129 were classified as cD/D in Schombert (1987ApJS...64..643S 1987ApJS...64..643S); NGC 7012, ESO 146-028, ESO 346-003, ESO 202-043, NGC 3842, PGC 026269 and IC 1634 were classified as cD/D in the NED notes by previous observations. Note (2): Search method code as follows: 1 = WHT 2 = Gemini - N2006B 3 = Gemini - S2006B 4 = Gemini - N2007A 5 = Gemini - S2007A 6 = Gemini - S2007B -------------------------------------------------------------------------------- Byte-by-byte Description of file: rv/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.2 arcsec Rad [-50/50] Radius 8- 12 I5 km/s RV ? Radial velocity 14- 15 I2 km/s e_RV ? rms uncertainty on RV 17- 19 I3 km/s sigma ? Velocity dispersion 21- 22 I2 km/s e_sigma ? rms uncertainty on sigma -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 30-Mar-2009
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