CDS

2007MNRAS.381.1463N

Query : 2007MNRAS.381.1463N

2007MNRAS.381.1463N - Mon. Not. R. Astron. Soc., 381, 1463-1472 (2007/November-2)

The high-mass end of the Tully-Fisher relation.

NOORDERMEER E. and VERHEIJEN M.A.W.

Abstract (from CDS):

We study the location of massive disc galaxies on the Tully-Fisher (TF) relation. Using a combination of K-band photometry and high-quality rotation curves, we show that in traditional formulations of the TF relation (using the width of the global HI profile or the maximum rotation velocity), galaxies with rotation velocities larger than 200km/s lie systematically to the right of the relation defined by less massive systems, causing a characteristic `kink' in the relations. Massive, early-type disc galaxies in particular have a large offset, up to 1.5 mag, from the main relation defined by less massive and later-type spirals.

The presence of a change in slope at the high-mass end of the TF relation has important consequences for the use of the TF relation as a tool for estimating distances to galaxies or for probing galaxy evolution. In particular, the luminosity evolution of massive galaxies since z ~ 1 may have been significantly larger than estimated in several recent studies.

We also show that many of the galaxies with the largest offsets have declining rotation curves and that the change in slope largely disappears when we use the asymptotic rotation velocity as kinematic parameter. The remaining deviations from linearity can be removed when we simultaneously use the total baryonic mass (stars + gas) instead of the optical or near-infrared luminosity. Our results strengthen the view that the TF relation fundamentally links the mass of dark matter haloes with the total baryonic mass embedded in them.


Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS

Journal keyword(s): galaxies: elliptical and lenticular, cD - galaxies: fundamental parameters - galaxies: kinematics and dynamics - galaxies: spiral - galaxies: statistics

Simbad objects: 50

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Number of rows : 50
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 NGC 338 GiG 01 00 36.4009452192 +30 40 08.278129992   14.0       ~ 97 1
2 NGC 1167 LIN 03 01 42.3322774176 +35 12 20.300948892   13.84 12.77     ~ 336 2
3 NGC 1324 LIN 03 25 01.6816298256 -05 44 44.975701104   14   12.31   ~ 59 0
4 UGC 2849 GiG 03 45 32.9196164448 +44 51 17.423865180   17       ~ 23 0
5 UGC 2916 G 04 02 33.9170114400 +71 42 21.124283292   14.9       ~ 58 2
6 IC 356 IG 04 07 46.8869589504 +69 48 44.715725208   13.3       ~ 140 1
7 UGC 3205 G 04 56 14.8692530064 +30 03 08.201990520   16.0       ~ 61 0
8 NGC 2273 Sy2 06 50 08.6691789600 +60 50 44.864645136   14.50 13.54     ~ 509 3
9 UGC 3580 G 06 55 30.9694563864 +69 33 47.319499836   13.01 12.57 12.08 11.50 ~ 92 1
10 UGC 3993 GiG 07 55 43.7634883752 +84 55 35.337706284   14.0       ~ 28 1
11 NGC 2599 Q? 08 32 11.3215409472 +22 33 38.005300296   13.4       ~ 109 1
12 ESO 563-21 EmG 08 47 16.981 -20 02 08.38   13.5   12.47 12.7 ~ 80 0
13 NGC 2654 SyG 08 49 11.8211394432 +60 13 16.366909476   12.80       ~ 134 0
14 NGC 2862 SyG 09 24 55.1049981312 +26 46 28.778156544   13.80       ~ 74 0
15 NGC 2955 GiG 09 41 16.6170758448 +35 52 56.147040624   13.90       ~ 101 0
16 NGC 2985 Sy1 09 50 22.233 +72 16 43.13   11.37 10.61     ~ 242 1
17 UGC 6399 G 11 23 23.2200537264 +50 53 33.503083728   14.9       ~ 103 0
18 UGC 6446 GiC 11 26 40.4656762968 +53 44 48.012539280   14.5       ~ 151 0
19 NGC 3726 GiG 11 33 21.1367545656 +47 01 45.280222428   11.11   10.02   ~ 345 0
20 NGC 3729 GiP 11 33 49.321 +53 07 31.79   12.2       ~ 195 1
21 UGC 6667 GiC 11 42 26.309 +51 35 52.82   14.8       ~ 114 0
22 NGC 3877 GiG 11 46 07.782 +47 29 40.20   11.8       ~ 314 0
23 NGC 3900 GiP 11 49 09.4563144120 +27 01 19.276393872   12.5       ~ 176 0
24 NGC 3898 LIN 11 49 15.370 +56 05 03.66   11.7       ~ 294 1
25 NGC 3917 GiP 11 50 45.4481861760 +51 49 27.919475076   12.5       ~ 180 0
26 NGC 3949 GiG 11 53 41.7311041896 +47 51 31.401451476   10.9       ~ 325 1
27 NGC 3953 GiG 11 53 49.0086582552 +52 19 36.475395312   11.08   9.71   ~ 345 0
28 UGC 6917 GiG 11 56 28.773 +50 25 42.22   14.0       ~ 132 0
29 M 109 GiG 11 57 35.9631479640 +53 22 29.006082336   10.94   9.57   ~ 441 0
30 NGC 4013 GiG 11 58 31.417 +43 56 49.28   12.4       ~ 413 1
31 NGC 4010 GiG 11 58 37.991 +47 15 40.72   13.1       ~ 145 0
32 UGC 6983 GiC 11 59 08.734 +52 42 28.03   14.5       ~ 167 0
33 NGC 4085 GiP 12 05 22.7304442992 +50 21 10.608113412   13.93 12.83     ~ 178 0
34 NGC 4088 GiP 12 05 34.2230093952 +50 32 21.064017876   11.2       ~ 394 1
35 NGC 4100 GiG 12 06 08.602 +49 34 56.32   11.7       ~ 238 0
36 NGC 4102 LIN 12 06 23.115 +52 42 39.42   11.8       ~ 410 1
37 NGC 4138 Sy1 12 09 29.8011417048 +43 41 06.864140004 12.46 12.29 11.32 10.82   ~ 393 1
38 NGC 4157 GiP 12 11 04.365 +50 29 04.85 12.48 12.15 11.35     ~ 340 2
39 NGC 4183 GiG 12 13 16.860 +43 41 53.77   13.5       ~ 191 0
40 NGC 4217 GiG 12 15 50.900 +47 05 30.44   12.4       ~ 289 2
41 IC 4202 EmG 13 08 31.5891545640 +24 42 02.857607676   15.2       ~ 97 0
42 NGC 5289 GiP 13 45 08.7075916440 +41 30 12.218593392   14.09 13.09     ~ 127 1
43 NGC 5533 Sy2 14 16 07.7507477232 +35 20 37.879981584   13.0       ~ 166 1
44 NAME Ursa Major Cluster ClG 15 08.8 +67 07           ~ 407 0
45 NGC 6195 LIN 16 36 32.5656632424 +39 01 40.411487460   14.7       ~ 91 0
46 UGC 11455 GiP 19 29 56.3064378840 +72 06 46.537706664   15.3       ~ 56 0
47 NGC 7013 G 21 03 33.5698770000 +29 53 50.926694208   12.9       ~ 134 0
48 UGC 11852 G 21 55 59.3494136184 +27 53 54.073166136   15.0       ~ 48 0
49 NGC 7217 LIN 22 07 52.3984675584 +31 21 33.632293572   12.94 11.92     ~ 482 0
50 NGC 7286 G 22 27 50.522 +29 05 45.57   13.4       ~ 45 0

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2023.05.29-17:29:55

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