CDS

2017A&A...607A..81B

Query : 2017A&A...607A..81B

2017A&A...607A..81B - Astronomy and Astrophysics, volume 607A, 81-81 (2017/11-1)

The concentration-mass relation of clusters of galaxies from the OmegaWINGS survey.

BIVIANO A., MORETTI A., PACCAGNELLA A., POGGIANTI B.M., BETTONI D., GULLIEUSZIK M., VULCANI B., FASANO G., D'ONOFRIO M., FRITZ J. and CAVA A.

Abstract (from CDS):

Context. The relation between a cosmological halo concentration and its mass (cMr) is a powerful tool to constrain cosmological models of halo formation and evolution.
Aims. On the scale of galaxy clusters the cMr has so far been determined mostly with X-ray and gravitational lensing data. The use of independent techniques is helpful in assessing possible systematics. Here we provide one of the few determinations of the cMr by the dynamical analysis of the projected-phase-space distribution of cluster members.
Methods. Based on the WINGS and OmegaWINGS data sets, we used the Jeans analysis with the MAMPOSSt technique to determine masses and concentrations for 49 nearby clusters, each of which has ≥60 spectroscopic members within the virial region, after removal of substructures.
Results. Our cMr is in statistical agreement with theoretical predictions based on ΛCDM cosmological simulations. Our cMr is different from most previous observational determinations because of its flatter slope and lower normalization. It is however in agreement with two recent cMr obtained using the lensing technique on the CLASH and LoCuSS cluster data sets.
Conclusions. The dynamical study of the projected-phase-space of cluster members is an independent and valid technique to determine the cMr of galaxy clusters. Our cMr shows no tension with theoretical predictions from ΛCDM cosmological simulations for low-redshift, massive galaxy clusters. In the future we will extend our analysis to galaxy systems of lower mass and at higher redshifts.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: clusters: general - galaxies: kinematics and dynamics - galaxies: kinematics and dynamics

VizieR on-line data: <Available at CDS (J/A+A/607/A81): table1.dat>

Simbad objects: 51

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Number of rows : 51
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022 		#notes
1 ACO 2717 ClG 00 03 12.9 -35 56 13           ~ 129 0
2 ACO 2734 ClG 00 11 21.60 -28 51 16.6           ~ 133 0
3 ACO 85 ClG 00 41 37.8 -09 20 33           ~ 839 0
4 ACO 119 ClG 00 56 16.8 -01 15 00           ~ 534 2
5 ACO 151 ClG 01 08 52.3 -15 25 01           ~ 183 1
6 ACO 160 ClG 01 12 59.572 +15 29 28.65           ~ 167 0
7 ACO 168 ClG 01 15 09.8 +00 14 51           ~ 344 2
8 ACO 193 ClG 01 25 07.3 +08 41 36           ~ 179 0
9 ACO 376 ClG 02 45 48 +36 51.6           B8.5 147 1
10 ACO 3128 ClG 03 30 34.6 -52 33 12           ~ 171 3
11 ACO 3158 ClG 03 42 39.6 -53 37 50           ~ 280 0
12 ACO 3266 ClG 04 31 11.9 -61 24 23           ~ 382 0
13 ACO 500 ClG 04 38 55.0 -22 05 55           ~ 77 0
14 ACO 3376 ClG 06 01 25.000 -39 59 51.00           ~ 284 0
15 ACO 3395 ClG 06 27 31.1 -54 23 58           ~ 188 0
16 ACO 671 ClG 08 28 31.97 +30 24 19.7           ~ 152 0
17 ACO 754 ClG 09 08 50.1 -09 38 12           ~ 643 1
18 ZwCl 0959+3257 ClG 10 02 23.39 +32 40 59.5           ~ 34 0
19 ACO 957 ClG 10 13 38.42 -00 55 32.6           ~ 200 2
20 ACO 970 ClG 10 17 34.3 -10 42 01           ~ 81 0
21 ACO 1069 ClG 10 39 54.3 -08 36 40           ~ 106 1
22 ClG J1216-1201 ClG 12 16 45.10 -12 01 17.3           ~ 66 0
23 ACO 1631 ClG 12 52 50.6 -15 25 37           ~ 167 1
24 ACO 3528 ClG 12 54 18.2 -29 01 16           ~ 150 1
25 ACO 3530 ClG 12 55 36 -30 21.2           ~ 92 0
26 ACO 1644 ClG 12 57 11.6 -17 24 34           ~ 343 1
27 ACO 3532 ClG 12 57 19.2 -30 22 13           ~ 160 2
28 ACO 3556 ClG 13 24 06.2 -31 39 38           ~ 142 0
29 ACO 3558 ClG 13 27 54.8 -31 29 32           ~ 417 2
30 ACO 3560 ClG 13 32 23.7 -33 08 21           ~ 124 1
31 ACO 1795 ClG 13 49 00.5 +26 35 07           ~ 1201 0
32 ACO 1983 ClG 14 52 44.0 +16 44 46           ~ 237 1
33 ACO 1991 ClG 14 54 30.2 +18 37 51           ~ 315 1
34 NAME NGC 5920 Group ClG 15 21 50.7 +07 42 18     15.13     ~ 295 0
35 ACO 2107 ClG 15 39 47.9 +21 46 21           ~ 240 0
36 ACO 2124 ClG 15 44 59.3 +36 03 40           ~ 197 0
37 ZwCl 1810+4949 ClG 18 11 00.1 +49 54 40     14.8     ~ 49 0
38 ACO 3667 ClG 20 12 33.68 -56 50 26.3           ~ 590 1
39 ACO 3716 ClG 20 51 16.7 -52 41 43           ~ 110 1
40 ZW II 108 BiC 21 13 55.918 +02 33 55.39   15.1       ~ 53 1
41 ACO 3809 ClG 21 46 57.5 -43 54 06           ~ 86 0
42 ACO 2382 ClG 21 51 57.2984 -15 36 48.067           ~ 112 0
43 ACO 2399 ClG 21 57 27.64 -07 48 12.9           ~ 175 0
44 ACO 2415 ClG 22 05 25.0 -05 35 23           ~ 109 1
45 ACO 3880 ClG 22 27 49.5 -30 34 40           ~ 90 2
46 ACO 2457 ClG 22 35 40.30 +01 31 33.6           ~ 124 0
47 ZwCl 2307+0713 ClG 23 10 26.6 +07 35 13           ~ 27 0
48 ACO 2589 ClG 23 24 00.5 +16 49 29           ~ 303 1
49 ACO 2593 ClG 23 24 31.0 +14 38 29           ~ 204 0
50 ACO 2626 ClG 23 36 31.0 +21 09 36           ~ 226 0
51 ACO 4059 ClG 23 56 40.7 -34 40 18           ~ 366 1

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2022.05.28-15:58:31

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