SIMBAD references

2018AstBu..73..124K - Astrophys. Bull., 73, 124-141 (2018/April-0)

Surveying the Local Supercluster Plane.

KASHIBADZE O.G., KARACHENTSEV I.D. and KARACHENTSEVA V.E.

Abstract (from CDS):

We investigate the distribution and velocity field of galaxies situated in a band of 100 by 20 degrees centered on M87 and oriented along the Local supercluster plane. Our sample amounts 2158 galaxies with radial velocities less than 2000 km s-1. 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 500-1000 km s-1 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 -840 km s-1. This cloud (or filament?) resides at a distance of 16.1 Mpc from us and approximately 5 Mpc away from the Virgo center. Galaxies around Virgo cluster exhibit Virgocentric infall with an amplitude of about 500 km s-1. Assuming the spherically symmetric radial infall, we estimate the radius of the zero-velocity surface to be R 0 = (7.0?0.3) Mpc that yields the total mass of Virgo cluster to be (7.4 ? 0.9)? 1014M? 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.

Abstract Copyright:

Journal keyword(s): galaxies: kinematics and dynamics - galaxies: distances and redshifts - galaxies: groups

VizieR on-line data: <Available at CDS (J/other/AstBu/73.124): lsci.dat>

Simbad objects: 2158

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2021.05.08-10:49:04

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