/ftp/cats/A+A/448//155



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J/A+A/448/155     Radial velocities of Leo I globular clusters  (Bergond+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	tablea[123].dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/448/155
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drwxr-xr-x 18 cats archive 325 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 315 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 476 Dec 19 2022 .message -r--r--r-- 1 cats archive 4570 Jun 4 2006 ReadMe -rw-r--r-- 1 cats archive 613 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2515 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1413 Mar 10 2006 tablea1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1079 Mar 10 2006 tablea2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 535 Mar 10 2006 tablea3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/448/155 Radial velocities of Leo I globular clusters (Bergond+, 2006) ================================================================================ Wide-field kinematics of globular clusters in the Leo I group. Bergond G., Zepf S.E., Romanowsky A.J., Sharples R.M., Rhode K.L. <Astron. Astrophys., 448, 155-164 (2006)> =2006A&A...448..155B ================================================================================ ADC_Keywords: Galaxies, nearby ; Clusters, globular ; Velocity dispersion ; Radial velocities ; Spectroscopy Keywords: galaxies: elliptical and lenticular, cD - galaxies: halos - galaxies: kinematics and dynamics - galaxies: star clusters Abstract: VLT/FLAMES radial velocities for 50 Globular Clusters (GCs), 37 field stars and 21 unclassified objects around the Leo I group galaxies NGC 3379 and NGC 3384 are presented. Object Id and BVR photometry are from Rhode & Zepf (2004AJ....127..302R). Positions (J2000.0) should be accurate to  0"2 or better w.r.t. the GSC2.1 catalogue. Heliocentric radial velocities and their errors were estimated by fitting the peak (see the width, heigh, and Tonry & Davies (1979AJ.....84.1511T) coefficient) of the cross-correlation function (CCF) with the IRAF/RV package task FXCOR, using simulatenous and ELODIE library stellar templates. Objects have been assigned three quality class, class A being the most secure velocity determination, and class C the least secure; the latter objects require confirmation, and such GCs were not considered for the dynamical analysis presented in the paper. Description: The FLAMES observations were carried out in service mode on VLT/UT2 (Kueyen), with the GIRAFFE/MEDUSA configuration. Our observing programme consisted of five 2595-s exposures taken on separate nights, in May-June 2003, under good seeing ( 0.7") conditions.