2004ApJ...613..866K


Query : 2004ApJ...613..866K

2004ApJ...613..866K - Astrophys. J., 613, 866-885 (2004/October-1)

Hα morphologies and environmental effects in Virgo cluster spiral galaxies.

KOOPMANN R.A. and KENNEY J.D.P.

Abstract (from CDS):

We describe the various Hα morphologies of Virgo Cluster and isolated spiral galaxies and associate the Hα morphologies with the types of environmental interactions that have altered the cluster galaxies. The spatial distributions of Hα and R-band emission are used to divide the star formation morphologies of the 52 Virgo Cluster spiral galaxies into several categories: normal (37%), anemic (6%), enhanced (6%), and (spatially) truncated (52%). Truncated galaxies are further subdivided on the basis of their inner star formation rates into truncated/normal (37%), truncated/compact (6%), truncated/anemic (8%), and truncated/enhanced (2%). The fraction of anemic galaxies is relatively small (6%-13%) in both environments, suggesting that starvation is not a major factor in the reduced star formation rates of Virgo spiral galaxies. The majority of Virgo spiral galaxies have their Hα disks truncated (52%), whereas truncated Hα disks are rarer in isolated galaxies (12%). Most of the Hα-truncated galaxies have relatively undisturbed stellar disks and normal to slightly enhanced inner disk star formation rates, suggesting that intracluster medium-interstellar medium (ICM-ISM) stripping is the main mechanism causing the reduced star formation rates of Virgo spiral galaxies. Several of the truncated galaxies are peculiar, with enhanced central star formation rates, disturbed stellar disks, and barlike distributions of luminous H II complexes inside the central 1 kpc but no star formation beyond, suggesting that recent tidal interactions or minor mergers have also influenced their morphology. Two highly inclined Hα-truncated spiral galaxies have numerous extraplanar H II regions and are likely in an active phase of ICM-ISM stripping. Several spiral galaxies have one-sided Hα enhancements at the outer edge of their truncated Hα disks, suggesting modest local enhancements in their star formation rates due to ICM-ISM interactions. Low-velocity tidal interactions and perhaps outer cluster H I accretion seem to be the triggers for enhanced global star formation in four Virgo galaxies. These results indicate that most Virgo spiral galaxies experience ICM-ISM stripping, many experience significant tidal effects, and many experience both.

Abstract Copyright: ∼

Journal keyword(s): Galaxies: Clusters: General - Galaxies: Clusters: Individual: Name: Virgo - Galaxies: Fundamental Parameters - Galaxies: Peculiar - Galaxies: Spiral - Galaxies: Structure

Simbad objects: 74

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Number of rows : 74
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 ZwCl 0024+1652 ClG 00 26 35.6 +17 09 32     18.35     ~ 648 1
2 NGC 613 AGN 01 34 18.235 -29 25 06.56   10.77 12.71 9.50 10.6 ~ 446 3
3 IC 356 AG? 04 07 46.8869589504 +69 48 44.715725208   13.3       ~ 161 1
4 NGC 1569 rG 04 30 49.186 +64 50 52.52 11.72 11.86 11.03     ~ 1297 3
5 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
6 NGC 4064 GiG 12 04 11.191 +18 26 36.42   12.5       ~ 186 0
7 NGC 4178 H2G 12 12 46.443 +10 51 57.59   12.9       ~ 367 0
8 NGC 4189 GiC 12 13 47.2380839784 +13 25 29.445094632   12.51 11.74     ~ 294 1
9 M 98 LIN 12 13 48.2910686976 +14 54 01.953475200 11.25 10.95 10.14     ~ 499 2
10 NGC 4212 H2G 12 15 39.3368219184 +13 54 05.388525900   11.9       ~ 328 0
11 NGC 4237 AGN 12 17 11.4198657984 +15 19 26.557164264   12.3       ~ 266 0
12 M 99 H2G 12 18 49.625 +14 24 59.36 10.45 10.44 9.87     ~ 1004 2
13 NGC 4262 GiG 12 19 30.5694336288 +14 52 39.517143276 13.00 12.49 11.55     ~ 378 1
14 NGC 4293 LIN 12 21 12.891 +18 22 56.64   11.6       ~ 311 2
15 NGC 4294 GiC 12 21 17.787 +11 30 39.99   12.6       ~ 320 0
16 NGC 4298 GiC 12 21 32.7578814360 +14 36 22.048690716   12.04 11.34     ~ 358 1
17 NGC 4299 GiC 12 21 40.548 +11 29 59.74   12.8       ~ 271 0
18 M 61 Sy2 12 21 54.9282582888 +04 28 25.597367184 10.07 10.18 9.65     ~ 1084 1
19 M 100 AGN 12 22 54.9299993592 +15 49 20.296257960 10.04 10.05 9.35     ~ 1963 2
20 NGC 4351 GiG 12 24 01.560 +12 12 18.09   13.5       ~ 239 0
21 NGC 4365 GiG 12 24 28.228 +07 19 03.07   11.5       ~ 871 0
22 MCG+03-32-027 GiC 12 25 21.618 +16 25 46.87   16.0       ~ 44 0
23 NGC 4380 BLL 12 25 22.178 +10 01 00.14   13.4       ~ 275 0
24 M 85 GiP 12 25 24.053 +18 11 27.89   10.2       ~ 678 0
25 NGC 4383 AGN 12 25 25.51753 +16 28 12.0180 12.41 12.67 12.12     ~ 274 2
26 NGC 4394 GiP 12 25 55.6366312872 +18 12 50.110707636   11.9       ~ 379 0
27 NGC 4405 H2G 12 26 07.1372151528 +16 10 51.581577504   13.03       ~ 169 1
28 M 86 GiG 12 26 11.814 +12 56 45.49 10.32 9.83 8.90   7.50 ~ 1126 1
29 NGC 4413 GiP 12 26 32.2311385872 +12 36 38.426455080   13.6 12.25     ~ 252 1
30 NGC 4411B Sy2 12 26 47.2270744440 +08 53 04.479254880   14.4       ~ 190 0
31 NGC 4419 LIN 12 26 56.4505296720 +15 02 50.688833388 12.42 12.08 11.16     ~ 419 2
32 NGC 4424 H2G 12 27 11.5741235616 +09 25 14.330453700   13.1       ~ 407 0
33 NGC 4438 LIN 12 27 45.6705493536 +13 00 31.708096380 11.37 11.02 10.17     ~ 668 2
34 NGC 4450 LIN 12 28 29.5910654016 +17 05 05.976112020   10.90 10.08     ~ 587 2
35 IC 3392 GiC 12 28 43.2764753520 +14 59 57.963302232   13.3       ~ 181 0
36 NGC 4457 LIN 12 28 59.0252479200 +03 34 14.215556928   11.9       ~ 342 0
37 M 49 Sy2 12 29 46.8 +08 00 01   13.21 12.17     ~ 2174 2
38 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
39 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
40 NGC 4498 GiG 12 31 39.5627385744 +16 51 09.625381632   12.8       ~ 244 0
41 M 88 Sy2 12 31 59.1525062448 +14 25 13.148971824   14.33 13.18     ~ 843 1
42 NGC 4519 GiG 12 33 30.278 +08 39 16.06   12.8       ~ 295 0
43 NGC 4522 GiG 12 33 39.657 +09 10 29.54   13.6       ~ 396 0
44 NGC 4527 AGN 12 34 08.49600 +02 39 13.7160   12.4       ~ 549 2
45 NGC 4532 H2G 12 34 19.329 +06 28 03.73   12.3       ~ 304 2
46 NGC 4535 H2G 12 34 20.3443516704 +08 11 51.908488116   11.1       ~ 679 0
47 NGC 4536 H2G 12 34 27.12887 +02 11 16.3680 11.14 11.16 10.55 17.393   ~ 913 3
48 Z 42-163 GiP 12 34 44.934 +06 17 59.58   15.3       ~ 116 1
49 M 91 LIN 12 35 26.4446761320 +14 29 46.760333748   14.63 13.57     ~ 639 0
50 NGC 4550 GiP 12 35 30.5913588048 +12 13 14.921166792 12.97 12.56 11.68     ~ 558 1
51 NGC 4561 GiG 12 36 08.137 +19 19 21.32   12.7       ~ 211 0
52 NGC 4567 H2G 12 36 32.6979947472 +11 15 28.716262668 12.25 12.06 11.31     ~ 339 2
53 NGC 4568 H2G 12 36 34.292 +11 14 19.07   12.11 11.19     ~ 394 2
54 M 90 Sy2 12 36 49.8009839880 +13 09 46.523813040 10.56 10.26 9.54     ~ 953 1
55 NGC 4571 GiC 12 36 56.3722998960 +14 13 02.296534836   13.6       ~ 368 1
56 M 58 Sy2 12 37 43.59747 +11 49 05.1240 10.80 10.48 9.66     ~ 1140 2
57 NGC 4580 LIN 12 37 48.3754581432 +05 22 06.630315636   13.1       ~ 233 0
58 NGC 4606 GiP 12 40 57.557 +11 54 43.87   12.7       ~ 173 0
59 NGC 4607 GiC 12 41 12.407 +11 53 11.86   14.7       ~ 184 0
60 NGC 4639 Sy1 12 42 52.3785000336 +13 15 26.706153600   13.62 12.72     ~ 642 0
61 NGC 4643 LIN 12 43 20.1435647088 +01 58 41.716062264   11.9       ~ 286 0
62 NGC 4647 H2G 12 43 32.542 +11 34 56.89   12.5 12.5     ~ 423 1
63 NGC 4651 LIN 12 43 42.6376070448 +16 23 36.002649300   11.30 10.92 10.42 9.84 ~ 537 0
64 NGC 4654 H2G 12 43 56.638 +13 07 34.86   11.8       ~ 600 1
65 NGC 4689 H2G 12 47 45.5568088416 +13 45 46.135889100   12.8       ~ 418 0
66 LEDA 43211 LSB 12 47 59.92392 +10 58 14.8966   21       ~ 83 0
67 NGC 4694 AGN 12 48 15.091 +10 59 01.05   13.93 13.36     ~ 302 0
68 NGC 4698 Sy2 12 48 22.9082830584 +08 29 14.667552276   13.24 12.27     ~ 507 0
69 NGC 4710 H2G 12 49 38.958 +15 09 55.76   11.6       ~ 329 0
70 NGC 4713 GiG 12 49 57.8802780576 +05 18 40.933127196   12.3       ~ 320 1
71 NGC 4772 LIN 12 53 29.1636448512 +02 10 06.146331708 12.29 11.96 11.04     ~ 265 1
72 NGC 4808 GiG 12 55 48.940 +04 18 14.74   12.5       ~ 244 1
73 NGC 4984 Sy1 13 08 57.2555329728 -15 30 58.743722520   12   10.92   ~ 142 0
74 IC 5273 EmG 22 59 26.719 -37 42 10.36   11.90 11.45 11.07 11.6 ~ 153 0

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