CDS

2019MNRAS.490.5017B

Query : 2019MNRAS.490.5017B

2019MNRAS.490.5017B - Mon. Not. R. Astron. Soc., 490, 5017-5032 (2019/December-3)

The rotational profiles of cluster galaxies.

BILTON L.E., HUNT M., PIMBBLET K.A. and ROEDIGER E.

Abstract (from CDS):

We compile two samples of cluster galaxies with complimentary hydrodynamic and N-body analysis using FLASH code to ascertain how their differing populations drive their rotational profiles and to better understand their dynamical histories.We select our main cluster sample from the X-ray Galaxy Clusters Database (BAX), which are populated with Sloan Digital Sky Survey (SDSS) galaxies. The BAX clusters are tested for the presence of substructures, acting as proxies for core mergers, culminating in sub-samples of eight merging and 25 non-merging galaxy clusters. An additional sample of 12 galaxy clusters with known dumbbell components is procured using galaxy data from the NASA/IPAC Extragalactic Database (NED) to compare against more extreme environments. BAX clusters of each sample are stacked on to a common RA-Dec. space to produce rotational profiles within the range of 0.0-2.5 r200. Merging stacks possess stronger core rotation at <=0.5r200 primarily contributed by a red galaxy sub-population from relaxing core mergers; this is alongside high rotational velocities from blue galaxy sub-populations, until they mix and homogenize with the red sub-populations at ∼r200, indicative of an infalling blue galaxy sub-population with interactive mixing between both sub-populations at >= r200. FLASH code is utilized to simulate the merger phase between two originally independent clusters and test the evolution of their rotational profiles. Comparisons with the dumbbell clusters leads to the inference that the peculiar core rotations of some dumbbell clusters are the result of the linear motions of core galaxies relaxing on to the potential during post second infall.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): galaxies: clusters: general - galaxies: elliptical and lenticular, cD - galaxies: kinematics and dynamics

Simbad objects: 47

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Number of rows : 47
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023 		#notes
1 ACO 85 ClG 00 41 37.8 -09 20 33           ~ 856 0
2 ACO 119 ClG 00 56 16.8 -01 15 00           ~ 543 2
3 ACO 2860 ClG 01 04.1 -39 47           ~ 22 0
4 ACO 2911 ClG 01 26 12.9 -37 56 22           ~ 63 0
5 ACO 426 ClG 03 19 47.2 +41 30 47           ~ 2149 1
6 ACO 3151 ClG 03 40 27.2 -28 40 20           ~ 42 0
7 ACO 3266 ClG 04 31 11.9 -61 24 23           ~ 397 0
8 ACO 533 ClG 05 01 30 -22 36.7           ~ 42 0
9 ACO 3391 ClG 06 26 15.4 -53 40 52           ~ 190 1
10 ACO 3395 ClG 06 27 31.1 -54 23 58           ~ 196 0
11 ACO 602 ClG 07 53 19.0 +29 22 27           ~ 71 0
12 ACO 1066 ClG 10 39 06.62 +05 12 35.2           ~ 88 1
13 ACO 1190 ClG 11 11 28.60 +40 49 48.0           ~ 120 0
14 ACO 1205 ClG 11 13 21.37 +02 32 39.4           ~ 67 0
15 ACO 1367 ClG 11 44 44.6 +19 41 59           ~ 1050 1
16 ZwCl 1215+0400 ClG 12 17 40.6 +03 39 45           ~ 118 0
17 ACO 1552 ClG 12 30 11.53 +11 44 37.9           ~ 95 0
18 ACO 1589 ClG 12 41 19.1 +18 34 16           ~ 97 0
19 ACO 3528 ClG 12 54 18.2 -29 01 16           ~ 153 1
20 ACO 3535 ClG 12 57 48 -28 29.2           ~ 21 2
21 ACO 1650 ClG 12 58 36.76 -01 43 34.2           ~ 290 0
22 ACO 1656 ClG 12 59 48.7 +27 58 50           ~ 4599 2
23 ACO 1668 ClG 13 03 44.90 +19 16 37.2           ~ 108 0
24 ACO 1750 ClG 13 30 49.94 -01 52 22.1           ~ 168 2
25 ACO 1767 ClG 13 36 08.33 +59 12 23.0           ~ 167 0
26 ACO 1773 ClG 13 42 11.73 +02 13 28.2           ~ 112 0
27 ACO 3570 ClG 13 46 50 -37 55.0           ~ 52 3
28 ACO 1795 ClG 13 49 00.5 +26 35 07           ~ 1220 0
29 ACO 1809 ClG 13 53 03.72 +05 08 17.7           ~ 166 0
30 ACO 1991 ClG 14 54 30.2 +18 37 51           ~ 318 1
31 ACO 2029 ClG 15 10 58.7 +05 45 42           ~ 909 0
32 ACO 2033 ClG 15 11 23.50 +06 19 08.4           ~ 92 0
33 ACO 2052 ClG 15 16 45.5 +07 00 01           ~ 709 1
34 ACO 2061 ClG 15 21 20.58 +30 40 15.3           ~ 179 1
35 ACO 2065 ClG 15 22 42.6 +27 43 21           ~ 358 0
36 ACO 2063 ClG 15 23 01.8 +08 38 22           ~ 387 2
37 ACO 2067 ClG 15 23 14 +30 54.4           ~ 104 1
38 ACO 2069 ClG 15 23 57.9 +29 53 26           ~ 133 0
39 ACO 2107 ClG 15 39 47.9 +21 46 21           ~ 245 0
40 ACO 2122 ClG 15 44 59.3 +36 03 40           ~ 219 0
41 ACO 2147 ClG 16 02 17.2 +15 53 43           ~ 395 0
42 ACO 2199 ClG 16 28 37.0 +39 31 28           ~ 1143 1
43 ACO 2255 ClG 17 12 50.04 +64 03 10.6           ~ 546 0
44 ACO 3653 ClG 19 53 14.4041 -52 03 59.306           ~ 24 0
45 ACO 3716 ClG 20 51 16.7 -52 41 43           ~ 111 1
46 ACO 3744 ClG 21 07 13.8 -25 28 54           ~ 75 1
47 ACO 2670 ClG 23 54 13.64 -10 25 08.7           ~ 347 0

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2023.01.28-10:44:12

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