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Home All issues Volume 515 (June 2010) A&A, 515 (2010) A57 Full HTML
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Table 1:

Heliocentric redshift, position, and morphological type for galaxies of A376, A970, A1356, and A2244.

Galaxy 		RA Dec Type Hel. Vel. R N
id. (2000) (2000)   $V \pm {\Delta}V$    
A376            
1 02 46 29.0 +36 27 19 S 40 451 32 6.53 1
4 02 46 21.0 +36 30 43 E 39 967 26 5.93 2
10 02 46 40.5 +36 35 44 S0 36 533 49 3.08  
12 02 46 25.4 +36 34 48 S0 13 881 59 3.98  
13 02 46 25.3 +36 32 24 S 15 026 61 5.69 l1
14 02 45 47.0 +36 35 57 S 13 526 127 3.05  
15 02 45 07.6 +36 36 49 S0 14 018 74 5.03  
16 02 45 06.7 +36 34 02 S 12 977 68 4.49 3
17 02 44 43.9 +36 35 46 E/S0 13 638 101 3.22  
19 02 46 47.6 +36 40 38 S0 13 629 108 3.01 weak
21 02 45 55.6 +36 43 14 S0 14 873 53 3.68 l2
23 02 45 32.6 +36 40 46 S 13 398 29 10.65 4
29 02 44 52.5 +36 40 21 S 15 602 68 3.35  
30 02 44 16.2 +36 44 00 S 41 071 50 3.79 5
38 02 46 25.0 +36 48 37 E 13 975 131 3.76  
39 02 46 20.5 +36 46 20 E/S0 15 415 100 3.39  
46 02 44 58.9 +36 45 54 S 14 401 49 4.25 l3
47 02 44 53.9 +36 47 32 Ep 14 514 60 3.29 l4
48 02 44 44.5 +36 45 00 I 14 702 56 6.69 6
50 02 44 11.1 +36 45 36 S0 29 935 61 4.25 l5
51 02 43 49.1 +36 46 30 S0/E 41 546 51 5.49  
53 02 47 31.8 +36 49 45 S 13 701 21 8.87  
56 02 46 54.5 +36 53 03 E 13 897 58 4.69 l6
58 02 46 34.2 +36 54 19 S 16 215 66 4.00 l7
59 02 46 28.3 +36 51 55 S 13 310 94 3.49  
62 02 46 19.7 +36 50 52 S/I 13 772 73   7
74 02 45 48.7 +36 52 28 S0 13 466 86 3.02 weak
77 02 45 41.1 +36 52 39 S 13 553 65 3.03  
79 02 45 33.5 +36 51 43 S0 14 184 119 3.19  
80 02 45 28.8 +36 53 33 S0 14 948 118 3.02  
82 02 45 22.6 +36 50 32 S0/S 26 848 58 3.73  
83 02 45 16.5 +36 50 45 S0 15 265 35 12.35 8
87 02 44 16.6 +36 54 49 S0 12 072 78 4.03 9
99 02 45 47.9 +36 59 09 S0 13 421 63 6.41  
105 02 45 09.4 +37 00 57 S0 13 550 98 3.81  
107 02 43 54.1 +36 57 49 E/S0 14 365 81 4.28  
110 02 45 41.9 +37 06 05 E 9255 49 5.96 l8
112 02 43 51.6 +37 03 30 S 13 535 88 2.54 weak
114 02 46 08.5 +37 09 49 S 13 260 98 3.04 10
115 02 44 56.2 +37 11 56 S 44 634 76 3.02  
116 02 44 14.2 +37 09 24 E/S0 40 204 75 5.16  
117 02 44 18.8 +37 08 20 S0 40 124 74 3.10  
118 02 45 38.4 +37 18 18 S 17 561 66 4.32 11
119 02 45 38.7 +37 18 25 S0/a 14 587 55 4.29 l9
120 02 45 07.8 +37 14 24 E 14 530 53 4.49  
A970            
70 10 16 05.3 -10 57 40 E 17 014 112 3.47  
71 10 16 08.0 -10 29 49 E/S0 11 033 91 5.70 12
72 10 16 10.8 -10 28 28 S0 55 419 77 2.96 weak
73 10 16 14.0 -10 31 13 S0 17 610 116 3.07 l10
74 10 16 25.7 -10 57 43 E/S0 18 009 154 3.01 l11
75 10 16 31.9 -10 37 45 S0 12 360 93 3.66 l12
76 10 16 39.8 -10 59 59 E 15 662 94 6.18 l13
77 10 16 41.3 -10 59 03 S0/S 47 793 60 3.04  
78 10 17 17.5 -11 07 50 S0 17 709 83 4.26  
79 10 18 53.9 -10 49 25 S 19 173 17   13
80 10 18 59.0 -10 54 02 E 2701 23   14
81 10 19 09.6 -10 58 39 S 19 404 32   15
82 10 19 13.7 -10 22 31 E 33 248 50 3.32  
83 10 19 16.2 -10 22 09 S0/S 16 887 111 3.01 weak
A1356            
1 11 42 04.8 +10 21 49 S 6395 43 5.19 l14
2 11 42 08.7 +10 27 19 S 21 030 82 3.63  
3 11 42 15.3 +10 26 50 E 35 166 27 11.75 l15
4 11 42 22.3 +10 44 19 S 23 753 45 8.93 l16
5 11 42 23.7 +10 26 09 E 21 474 54 6.96 16 l29
6 11 42 24.4 +10 40 04 S 23 794 79 6.70 l17
7 11 42 29.6 +10 29 24 S 20 910 75 6.27  
8 11 42 29.7 +10 28 31 S0 20 702 51 10.56 l18
9 11 42 31.7 +10 25 24 S 10 655 75 5.61 17 l30
10 11 42 43.4 +10 31 00 E 36 132 74 3.62 weak l31
A2244            
1 17 02 16.7 +33 58 49 S 29 626 39 10.37 l19
2 17 02 25.9 +33 59 54 S0 29 062 32 11.18 l20
3 17 02 42.5 +34 03 38 S0 29 811 46 9.50 l21
4 17 02 45.6 +34 03 39 ? 27 984 66 8.67 l22
5 17 03 23.5 +34 06 49 S 11 080 25 12.40 18 l23
6 17 04 03.3 +33 55 19 S 11 144 39 10.96 l24
7 17 04 04.1 +34 15 29 S0 30 606 73 6.83 l25
8 17 04 14.4 +34 15 03 S 12 180 80 6.39 19 l26
9 17 04 45.9 +34 06 34 S0 30 707 58 8.76 l27
10 17 04 50.1 +34 05 29 S 9959 58 7.29 20 l28

Notes. Data from NED:
l1  $15~130~{\rm km~s^{-1}}$; l2  $14~958~{\rm km~s^{-1}}$; l3  $14~590~{\rm km~s^{-1}}$; l4  $14~466~{\rm km~s^{-1}}$; l5  $29~892~{\rm km~s^{-1}}$; l6  $13~988~{\rm km~s^{-1}}$; l7  $16~273~{\rm km~s^{-1}}$; l8  $9324~{\rm km~s^{-1}}$; l9  $14~765~{\rm km~s^{-1}}$; l10  $17~631~{\rm km~s^{-1}}$; l11  $18~067~{\rm km~s^{-1}}$; l12  $12~098~{\rm km~s^{-1}}$; l13  $15~782~{\rm km~s^{-1}}$; l14 NGC 3819 $6274~{\rm km~s^{-1}}$; l15  $35~155~{\rm km~s^{-1}}$; l16  $23~768~{\rm km~s^{-1}}$; l17  $23~789~{\rm km~s^{-1}}$; l18  $20~773~{\rm km~s^{-1}}$; l19  $29~585~{\rm km~s^{-1}}$; l20  $29~046~{\rm km~s^{-1}}$; l21  $29~652~{\rm km~s^{-1}}$; l22  $27~955~{\rm km~s^{-1}}$; l23  $11~121~{\rm km~s^{-1}}$; l24  $11~156~{\rm km~s^{-1}}$; l25  $30~655~{\rm km~s^{-1}}$; l26  $12~110~{\rm km~s^{-1}}$; l27  $30~809~{\rm km~s^{-1}}$; l28  $9908~{\rm km~s^{-1}}$; l29  $21~288~{\rm km~s^{-1}}$; l30  $10~601~{\rm km~s^{-1}}$; l31  $36~047~{\rm km~s^{-1}}$.
1 emission line: ${\rm H}\alpha= 40~498~{\rm km~s^{-1}}$; 2 emission line: ${\rm H}\alpha= 39~982~{\rm km~s^{-1}}$; 3 emission line: ${\rm H}\alpha= 13~072~{\rm km~s^{-1}}$; 4 emission line: ${\rm H}\beta$, 2OIII, ${\rm H}\alpha, S2$; 5 emission line: ${\rm H}\alpha= 41~167~{\rm km~s^{-1}}$; 6 emission line: ${\rm H}\alpha= 14~829~{\rm km~s^{-1}}$; 7 emission line: OII, ${\rm H}\beta$, 2OIII, ${\rm H}\alpha, S1$; 8 emission line: ${\rm H}\alpha, S2= 15~478~{\rm km~s^{-1}}$; 9 emission line: ${\rm H}\alpha= 12~066~{\rm km~s^{-1}}$; 10 emission line: ${\rm H}\alpha= 13~267~{\rm km~s^{-1}}$; 11 emission line: ${\rm H}\alpha= 17~652~{\rm km~s^{-1}}$; 12 emission line: ${\rm H}\alpha= 11~058~{\rm km~s^{-1}}$; 13 emission line: ${\rm H}\alpha$; 14 emission lines: 2OIII, ${\rm H}\alpha, S1$; 15 emission line: ${\rm H}\alpha$; 16 emission lines: OII, OIII, ${\rm H}\alpha$, $N2= 21~398 \pm 68~{\rm km~s^{-1}}$; 17 emission lines: 2OIII, ${\rm H}\alpha= 10~684 \pm 35~{\rm km~s^{-1}}$; 18 emission lines: ${\rm H}\alpha, N2$; 19 emission line: ${\rm H}\alpha$; 20 emission lines: ${\rm H}\beta$, 2OIII, ${\rm H}\alpha, N1, N2, S1, S2$.


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