2015ApJ...805..144K


Query : 2015ApJ...805..144K

2015ApJ...805..144K - Astrophys. J., 805, 144 (2015/June-1)

Peculiar velocities of galaxies in the Leo spur.

KARACHENTSEV I.D., TULLY R.B., MAKAROVA L.N., MAKAROV D.I. and RIZZI L.

Abstract (from CDS):

The Hubble Space Telescope Advanced Camera for Surveys has been used to determine accurate distances for the spiral galaxy NGC 2683 and 12 other galaxies in a zone of the ''local velocity anomaly'' from luminosity measurements of the brightest red giant branch stars. These galaxies lie in the Leo Spur, the nearest filament beyond our Local Sheet. The new accurate distance measurements confirm that galaxies along the Leo Spur are more distant than expected from uniform cosmic expansion, and hence have large and peculiar velocities toward us. The motions are generally explained by a previously published model that posits that the Local Sheet is descending at 259 km/s toward the south supergalactic pole due to expansion of the Local Void and is being attracted toward the Virgo Cluster at 185 km/s. With the standard ΛCDM cosmology, an empty void expands at 16 km/s/Mpc, so a motion of 259 km/s requires the Local Void to be impressively large and empty. Small residuals from the published model can be attributed to an upward push toward the north supergalactic pole by the expansion of the Gemini-Leo Void below the Leo Spur. The Leo Spur is sparsely populated, but among its constituents there are two associations that contain only dwarf galaxies.

Abstract Copyright: ∼

Journal keyword(s): dark matter - galaxies: distances and redshifts - galaxies: dwarf - large-scale structure of universe

Simbad objects: 32

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Number of rows : 32
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 UGC 3600 LSB 06 55 39.81787 +39 05 43.7871   18       ~ 46 0
2 UGC 3698 AG? 07 09 18.75 +44 22 48.2   17       ~ 45 0
3 NGC 2337 rG 07 10 13.6374445464 +44 27 26.716619844   13.1       ~ 94 1
4 UGC 3775 AG? 07 15 52.60 +12 06 53.9   17       ~ 16 0
5 UGC 3817 G 07 22 44.48 +45 06 30.7   17       ~ 49 0
6 Z 206-10 AG? 07 28 17.724 +40 46 11.36   15.50       ~ 155 0
7 LEDA 5060050 G 07 36 10.3 +09 59 11           ~ 25 0
8 MCG+07-16-011 AG? 07 41 25.777 +40 06 46.05   16.0       ~ 125 0
9 Z 87-30 G 07 41 56.3059298112 +16 48 07.451632188   15.4       ~ 233 0
10 [KK98a] 073940.2+164047 G 07 42 31.2 +16 33 40   15.6       ~ 52 0
11 LEDA 5060076 AG? 07 50 21.70 +07 47 40.0           ~ 30 0
12 Z 88-7 G 07 57 01.027 +14 23 47.66   16.0       ~ 161 0
13 NGC 2541 GiG 08 14 40.1160678912 +49 03 42.021679932 12.03 12.26 11.80     ~ 333 1
14 MCG+07-18-004 LSB 08 28 28.560 +41 51 27.13   18       ~ 175 0
15 LEDA 4087020 AG? 08 51 12.114 +27 52 48.15           ~ 29 0
16 NGC 2683 AGN 08 52 41.3064829584 +33 25 18.597681516 11.57 10.68 9.79 9.38   ~ 475 1
17 LEDA 166095 G 08 52 50.8 +33 47 52   16.8       ~ 28 0
18 [KK98a] 70 G 08 55 22.0 +33 33 33   17.7       ~ 16 0
19 NGC 2841 LIN 09 22 02.6778711696 +50 58 35.737082868 10.43 10.09 9.22     ~ 1113 1
20 NGC 2903 AGN 09 32 10.111 +21 30 02.99 10.44 9.75 9.07 8.68   ~ 1204 3
21 UGC 5209 LSB 09 45 04.196 +32 14 16.03   19       ~ 66 0
22 UGC 5288 PaG 09 51 17.241 +07 49 32.05 15.07 14.65 14.18 13.99   ~ 95 0
23 Z 64-68 AG? 10 07 20.182 +10 21 40.16   13.78   13.24   ~ 125 0
24 NGC 3198 EmG 10 19 54.990 +45 32 58.88 10.83 10.87 10.33     ~ 946 1
25 LEDA 1824266 AG? 10 31 55.8039010320 +28 01 33.737319084           ~ 31 0
26 NAME Leo Cluster ClG 11 30.0 +15 00           ~ 71 0
27 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
28 NAME Local Supercluster SCG 12 31 +12.4           ~ 566 0
29 ACO 1656 ClG 12 59 44.40 +27 54 44.9           ~ 5141 2
30 NAME Local Void vid 18 38 +18.0           ~ 234 0
31 NAME Local Group GrG ~ ~           ~ 9325 0
32 NAME Leo Spur reg ~ ~           ~ 36 0

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