/ftp/cats/aliases/K/./KGK2007_2_



==========================================================================
J/AJ/134/566        Leo II stellar kinematics                (Koch+, 2007)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AJ/134/566
==========================================================================

drwxr-xr-x 57 cats archive 4096 Jul 9 2015 [Up] drwxr-xr-x 2 cats archive 266 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 461 Dec 19 2022 .message -r--r--r-- 1 cats archive 3669 Jan 12 2010 ReadMe -rw-r--r-- 1 cats archive 1012 Jan 12 2010 +footg5.gif -rw-r--r-- 1 cats archive 2936 Jan 12 2010 +footg8.gif -r--r--r-- 1 cats archive 10448 Sep 7 2009 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/134/566 Leo II stellar kinematics (Koch+, 2007) ================================================================================ Stellar kinematics in the remote Leo II dwarf spheroidal Galaxy. Another brick in the wall. Koch A., Kleyna J.T., Wilkinson M.I., Grebel E.K., Gilmore G.F., Evans N.W., Wyse R.F.G., Harbeck D.R. <Astron. J., 134, 566-578 (2007)> =2007AJ....134..566K ================================================================================ ADC_Keywords: Galaxies, nearby ; Velocity dispersion ; Abundances, [Fe/H] Keywords: galaxies: dwarf - galaxies: individual (Leo II) - galaxies: kinematics and dynamics - galaxies: stellar content - galaxies: structure - Local Group Abstract: We present the projected velocity dispersion profile for the remote (d=233kpc) Galactic dwarf spheroidal (dSph) galaxy Leo II, based on 171 discrete stellar radial velocities that were obtained from medium-resolution spectroscopy using the FLAMES/GIRAFFE spectrograph at the European Southern Observatory, Chile. Description: In the framework of the ESO Large Program 171.B-0520(A) (principal investigator: G.F. Gilmore), which aims to elucidate the kinematic and chemical characteristics of Galactic dSphs, five fields in Leo II were observed using the FLAMES multiobject facility at ESO's Very Large Telescope.