========================================================================== J/MNRAS/415/1188 Galaxies in the Lynx-Cancer void (Pustilnik+, 2011) The following files can be converted to FITS (extension .fit or fit.gz) table2.dat tablea1.dat tablea2.dat ========================================================================== Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/415/1188 ==========================================================================
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Beginning of ReadMe : J/MNRAS/415/1188 Galaxies in the Lynx-Cancer void (Pustilnik+, 2011) ================================================================================ Study of galaxies in the Lynx-Cancer void. I. Sample description. Pustilnik S.A., Tepliakova A.L. <Mon. Not. R. Astron. Soc., 415, 1188-1201 (2011)> =2011MNRAS.415.1188P ================================================================================ ADC_Keywords: Galaxies, nearby ; Redshifts ; Space velocities Keywords: galaxies: distances and redshifts - galaxies: dwarf - galaxies: evolution - galaxies: luminosity function, mass function - large-scale structure of Universe Abstract: The evolution of galaxies is influenced by the environment in which they reside. This effect should be strongest for the lowest-mass and lowest-luminosity galaxies. To study dwarf galaxies in extremely low density environments, we have compiled a deep catalogue of dwarf galaxies in the nearby Lynx-Cancer void. This void hosts some of the most metal-poor dwarfs known to date. It borders the Local Volume at negative supergalactic Z(SGZ) coordinates and has a size of more than 16Mpc. With a distance to its centre of only 18Mpc, it is close enough to allow a search for the faintest dwarfs. Within the void 75 dwarf (-11.9>M_B_>-18.0) and four subluminous (-18.0>M_B_>-18.4) galaxies have been identified. We present the parameters of the void galaxies and a detailed analysis of the completeness of the catalogue as a function of magnitude and surface brightness.