/ftp/cats/J_other/AstBu/73.124



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J/other/AstBu/73.124 Galaxies in the Local Supercluster band (Kashibadze+, 2018)
The following files can be converted to FITS (extension .fit or fit.gz)
	lsci.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/other/AstBu/73.124
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Beginning of ReadMe : J/other/AstBu/73.124 Galaxies in the Local Supercluster band (Kashibadze+, 2018) ================================================================================ Surveying the Local Supercluster Plane. Kashibadze O.G., Karachentsev I.D., Karachentseva V.E. <Astrophys. Bull., 73, 124-141 (2018)> =2018AstBu..73..124K (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Clusters, galaxy ; Redshifts Keywords: galaxies: clusters: individual: Virgo - galaxies: kinematics and dynamics - galaxies: distances and redshifts - galaxies: groups Abstract: We investigate the distribution and velocity field of galaxies situated in a band of 100x20 degrees centered on M87 and oriented along the Local supercluster plane. Our sample amounts 2158 galaxies with radial velocities less than 2000 km/s. Of them, 1119 galaxies (52%) have distance and peculiar velocity estimates. About 3/4 of early-type galaxies are concentrated within the Virgo cluster core, most of the late-type galaxies in the band locate outside the virial radius. Distribution of gas-rich dwarfs with M_HI_> M* looks to be insensitive to the Virgo cluster presence. Among 50 galaxy groups in the equatorial supercluster band 6 groups have peculiar velocities about 500-1000km/s comparable with virial motions in rich clusters. The most cryptic case is a flock of nearly 30 galaxies around NGC4278 (Coma I cloud), moving to us with the mean peculiar velocity of -840km/s. This cloud (or filament?) resides at a distance of 16.1Mpc from us and approximately 5Mpc away from the Virgo center. Galaxies around Virgo cluster exhibit Virgocentric infall with an amplitude of about 500 km/s. Assuming the spherically symmetric radial infall, we estimate the radius of the zero-velocity surface to be R0=(7.0+/-0.3)Mpc that yields the total mass of Virgo cluster to be (7.4+/-0.9)x10^14^ solar masses, in tight agreement with its virial mass estimates. We conclude that the Virgo outskirts does not contain significant amounts of dark mater beyond its virial core. Description: The list of 2158 galaxies with supergalactic coordinates SGL = [52.9, 152.9] degrees, SGB = [-12.4, +7.6] degrees and radial velocities V_LG_<2000km/s. 1119 galaxies have distance measurements.

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