2019ApJ...880...52A


Query : 2019ApJ...880...52A

2019ApJ...880...52A - Astrophys. J., 880, 52-52 (2019/July-3)

Peculiar velocities of Galaxies just beyond the Local Group.

ANAND G.S., TULLY R.B., RIZZI L., SHAYA E.J. and KARACHENTSEV I.D.

Abstract (from CDS):

The Milky Way lies in a thin plane, the Local Sheet, a part of a wall bounding the Local Void lying toward the north supergalactic pole. Galaxies with accurate distances both above and below this supergalactic equatorial plane have systematically negative peculiar velocities. The interpretation of this situation is that the Local Void is expanding, giving members of the Local Sheet deviant velocities toward the south supergalactic pole. The few galaxies within the void are evacuating the void. Galaxies in a filament in the supergalactic south are not feeling the expansion so their apparent motion toward us is mainly a reflex of our motion. The model of the local velocity field was uncertain because the apex of our motion away from the Local Void lies in obscurity near the Galactic plane. Here, results of Hubble Space Telescope infrared observations are reported that find tip of the red giant branch distances to four obscured galaxies. All the distances are ∼7 Mpc, revealing that these galaxies are part of a continuous filamentary structure passing between the north and south Galactic hemispheres and sharing the same kinematic signature of peculiar velocities toward us. A fifth galaxy nearby in projection, GALFA-DW4, has an ambiguous distance. If nearby at ∼3 Mpc, this galaxy has an anomalous velocity away from us of +348 km s–1. Alternatively, perhaps the resolved stars are on the asymptotic giant branch and the galaxy is beyond 6 Mpc whence the observed velocity would not be unusual.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: distances and redshifts - galaxies: stellar content - Hertzsprung-Russell and C-M diagrams - large-scale structure of universe

Simbad objects: 18

goto Full paper

goto View the references in ADS

Number of rows : 18
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 300 GiG 00 54 53.4465638304 -37 41 03.168402396 8.83 8.69 8.13 7.46   ~ 1614 2
2 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 2029 0
3 NAME NGC 1566 Group GrG 04 20 00.6 -54 56 17           ~ 180 0
4 NAME Ori Dwarf Galaxy GiC 05 45 01.6 +05 03 41   18.0       ~ 46 0
5 LEDA 5072715 G 05 45 44.79 +10 46 15.6           ~ 11 0
6 * alf Ori s*r 05 55 10.30536 +07 24 25.4304 4.38 2.27 0.42 -1.17 -2.45 M1-M2Ia-Iab 1789 0
7 [BCK2005] HIZSS003B GiP 07 00 24.5446 -04 13 12.463           ~ 8 0
8 LEDA 2807061 G 07 00 29.3 -04 12 30           ~ 43 1
9 PN K 2-3 PN 07 06 56.8 -22 02 26   15.8       ~ 51 0
10 LEDA 2807065 G 07 46 06.0 -28 25 36           ~ 12 0
11 NAME Great Attractor SCG 10 32 -46.0           ~ 617 0
12 M 96 GiP 10 46 45.744 +11 49 11.78 10.42 10.15 9.25 8.99   ~ 862 1
13 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
14 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 3138 2
15 NAME Local Void vid 18 38 +18.0           ~ 234 0
16 NGC 6946 H2G 20 34 52.332 +60 09 13.24   10.5       ~ 2661 2
17 NAME Local Group GrG ~ ~           ~ 9325 0
18 NAME Leo Spur reg ~ ~           ~ 36 0

To bookmark this query, right click on this link: simbad:objects in 2019ApJ...880...52A and select 'bookmark this link' or equivalent in the popup menu