2003MNRAS.339L...1M

Query : 2003MNRAS.339L...1M

2003MNRAS.339L...1M - Mon. Not. R. Astron. Soc., 339, L1-L5 (2003/February-2)

The Tully-Fisher relation of cluster spirals at z = 0.83.

MILVANG-JENSEN B., ARAGON-SALAMANCA A., HAU G.K.T., JORGENSEN I. and HJORTH J.

Abstract (from CDS):

We present the rest-frame B -band Tully-Fisher relation for a sample of 8 cluster spiral galaxies at z = 0.83 and 19 field spirals at z = 0.15-0.90 based on Very Large Telescope (VLT) spectroscopy and Hubble Space Telescope (HST) photometry. No strong difference is detected between the cluster and the field galaxies, but we find some evidence that the cluster spirals are ∼0.5-1 mag brighter than the field ones at a fixed rotation velocity. Although only a ∼1.5-2σ result, if confirmed with larger samples this effect could be caused by the cluster spirals experiencing a period of enhanced star formation while falling into the cluster.

Abstract Copyright: RAS

Journal keyword(s): galaxies: evolution - galaxies: clusters: individual: MS1054.4-0321 - galaxies: spiral

Nomenclature: Fig.1: [MAH2003] FNN (Nos F01-F22), [MAH2003] CNN (No. C01).

CDS comments: Fig.1: Galaxies numbered 'NNNN' are '[VFK98] NNNN' in SIMBAD.

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 [MAH2003] F02 G 10 56 48.3 -03 37 33           ~ 2 0
2 [MAH2003] F21 G 10 56 48.6 -03 35 42           ~ 2 0
3 [MAH2003] F19 G 10 56 50.7 -03 35 39           ~ 2 0
4 [FFL2006] 1316 GiC 10 56 51.298 -03 36 11.17           ~ 3 0
5 [MAH2003] F06 G 10 56 53.0 -03 38 41           ~ 2 0
6 [MAH2003] F14 G 10 56 54.7 -03 39 00           ~ 2 0
7 [MAH2003] F04 G 10 56 56.0 -03 37 28           ~ 2 0
8 [SSE2005] C-2-1503-4651 GiC 10 56 56.46 -03 39 10.1           ~ 5 0
9 [BVF2002] C1 GiC 10 56 59.66 -03 37 27.8           ~ 12 0
10 ClG 1054-03 ClG 10 57 00.2 -03 37 27     22     ~ 458 0
11 [MAH2003] F16 G 10 57 01.2 -03 34 20           ~ 2 0
12 [MAH2003] F05 G 10 57 01.3 -03 35 44           ~ 2 0
13 [MAH2003] F18 G 10 57 03.7 -03 38 33           ~ 2 0
14 [BVF2002] C5 GiC 10 57 03.87 -03 37 41.8           ~ 10 0
15 [HPM2006] MS 1054.4-0321 4101 GiC 10 57 03.876 -03 35 05.29       23.13   ~ 6 0
16 [MAH2003] F20 G 10 57 05.731 -03 36 25.09       23.22   ~ 3 0
17 [CWB2011] WLTV J105707.27-033538.6 bCG 10 57 07.269 -03 35 38.60       23.17   ~ 8 0
18 [MAH2003] F22 G 10 57 07.8 -03 37 04           ~ 2 0
19 [MAH2003] F08 G 10 57 08.2 -03 37 34           ~ 2 0
20 [SSE2005] D-3-1028-7337 GiC 10 57 08.3 -03 36 42           ~ 3 0
21 [MAH2003] F12 G 10 57 11.5 -03 36 44           ~ 2 0
22 [SSE2005] D-4-6558-5379 GiC 10 57 12.11 -03 36 48.9           ~ 4 1
23 [MAH2003] F10 G 10 57 12.3 -03 37 17           ~ 2 0
24 [MAH2003] F17 G ~ ~           ~ 1 0
25 [MAH2003] F15 G ~ ~           ~ 1 0
26 [MAH2003] F13 G ~ ~           ~ 1 0
27 [MAH2003] F09 G ~ ~           ~ 1 0
28 [MAH2003] F07 G ~ ~           ~ 1 0
29 [MAH2003] F03 G ~ ~           ~ 1 0
30 [MAH2003] F01 G ~ ~           ~ 1 0
31 [VFK98] 1801 GiC ~ ~           ~ 3 0
32 [VFK98] 1763 GiC ~ ~           ~ 2 0

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