Barred disks in dense environments

I. Marinova; S. Jogee; A. Heiderman; F. D. Barazza; M. E. Gray; M. Barden; C. Wolf; C. Y. Peng; D. Bacon; M. Balogh; E. F. Bell; A. Böhm; J. A.R. Caldwell; B. Häußler; C. Heymans; K. Jahnke; E. Van Kampen; K. Lane; D. H. McIntosh; K. Meisenheimer; S. F. Sánchez; R. Somerville; A. Taylor; L. Wisotzki; X. Zheng

Barred disks in dense environments

I. Marinova^*, S. Jogee, A. Heiderman, F. D. Barazza, M. E. Gray, M. Barden, C. Wolf, C. Y. Peng, D. Bacon, M. Balogh, E. F. Bell, A. Böhm, J. A.R. Caldwell, B. Häußler, C. Heymans, K. Jahnke, E. Van Kampen, K. Lane, D. H. McIntosh, K. MeisenheimerS. F. Sánchez, R. Somerville, A. Taylor, L. Wisotzki, X. Zheng

^*Corresponding author for this work

Research output: Contribution to journal › Conference article › peer-review

1 Citation (Scopus)

Abstract

We investigate the properties of bright barred and unbarred disks in the Abell 901/902 cluster system at z ∼ 0.165 with the STAGES HST ACS survey. We find that the global optical bar fraction in the clusters is ∼ 30% regardless of the method of disk selection. Within a given absolute magnitude bin, the bar fraction increases for galaxies with no significant bulge component. Within each morphological type bin, the bar fraction increases for brighter galaxies. We find no strong trend for the bar fraction with local density within the cluster between the core and virial radius. We discuss the implications of our results for the evolution of bars and disks in dense environments.

Original language	English
Pages (from-to)	61-67
Number of pages	7
Journal	Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society
Volume	18
Publication status	Published - 2011
Externally published	Yes
Event	Tumbling, Twisting and Winding Galaxies: Pattern Speeds Along the Hubble Sequence - Padova, Italy Duration: 25 Aug 2008 → 28 Aug 2008

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Marinova, I., Jogee, S., Heiderman, A., Barazza, F. D., Gray, M. E., Barden, M., Wolf, C., Peng, C. Y., Bacon, D., Balogh, M., Bell, E. F., Böhm, A., Caldwell, J. A. R., Häußler, B., Heymans, C., Jahnke, K., Van Kampen, E., Lane, K., McIntosh, D. H., ... Zheng, X. (2011). Barred disks in dense environments. Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society, 18, 61-67.

@article{278ea97a7bf24af5873080731d468ea3,

title = "Barred disks in dense environments",

abstract = "We investigate the properties of bright barred and unbarred disks in the Abell 901/902 cluster system at z ∼ 0.165 with the STAGES HST ACS survey. We find that the global optical bar fraction in the clusters is ∼ 30% regardless of the method of disk selection. Within a given absolute magnitude bin, the bar fraction increases for galaxies with no significant bulge component. Within each morphological type bin, the bar fraction increases for brighter galaxies. We find no strong trend for the bar fraction with local density within the cluster between the core and virial radius. We discuss the implications of our results for the evolution of bars and disks in dense environments.",

keywords = "Galaxies: clusters: individual: Abell 901/902, Galaxies: evolution",

author = "I. Marinova and S. Jogee and A. Heiderman and Barazza, {F. D.} and Gray, {M. E.} and M. Barden and C. Wolf and Peng, {C. Y.} and D. Bacon and M. Balogh and Bell, {E. F.} and A. B{\"o}hm and Caldwell, {J. A.R.} and B. H{\"a}u{\ss}ler and C. Heymans and K. Jahnke and {Van Kampen}, E. and K. Lane and McIntosh, {D. H.} and K. Meisenheimer and S{\'a}nchez, {S. F.} and R. Somerville and A. Taylor and L. Wisotzki and X. Zheng",

note = "Publisher Copyright: {\textcopyright} SAIt 2011.; Tumbling, Twisting and Winding Galaxies: Pattern Speeds Along the Hubble Sequence ; Conference date: 25-08-2008 Through 28-08-2008",

year = "2011",

language = "English",

volume = "18",

pages = "61--67",

journal = "Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society",

issn = "1824-016X",

publisher = "Societa Astronomica Italiana",

}

Marinova, I, Jogee, S, Heiderman, A, Barazza, FD, Gray, ME, Barden, M, Wolf, C, Peng, CY, Bacon, D, Balogh, M, Bell, EF, Böhm, A, Caldwell, JAR, Häußler, B, Heymans, C, Jahnke, K, Van Kampen, E, Lane, K, McIntosh, DH, Meisenheimer, K, Sánchez, SF, Somerville, R, Taylor, A, Wisotzki, L & Zheng, X 2011, 'Barred disks in dense environments', Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society, vol. 18, pp. 61-67.

TY - JOUR

T1 - Barred disks in dense environments

AU - Marinova, I.

AU - Jogee, S.

AU - Heiderman, A.

AU - Barazza, F. D.

AU - Gray, M. E.

AU - Barden, M.

AU - Wolf, C.

AU - Peng, C. Y.

AU - Bacon, D.

AU - Balogh, M.

AU - Bell, E. F.

AU - Böhm, A.

AU - Caldwell, J. A.R.

AU - Häußler, B.

AU - Heymans, C.

AU - Jahnke, K.

AU - Van Kampen, E.

AU - Lane, K.

AU - McIntosh, D. H.

AU - Meisenheimer, K.

AU - Sánchez, S. F.

AU - Somerville, R.

AU - Taylor, A.

AU - Wisotzki, L.

AU - Zheng, X.

PY - 2011

Y1 - 2011

N2 - We investigate the properties of bright barred and unbarred disks in the Abell 901/902 cluster system at z ∼ 0.165 with the STAGES HST ACS survey. We find that the global optical bar fraction in the clusters is ∼ 30% regardless of the method of disk selection. Within a given absolute magnitude bin, the bar fraction increases for galaxies with no significant bulge component. Within each morphological type bin, the bar fraction increases for brighter galaxies. We find no strong trend for the bar fraction with local density within the cluster between the core and virial radius. We discuss the implications of our results for the evolution of bars and disks in dense environments.

AB - We investigate the properties of bright barred and unbarred disks in the Abell 901/902 cluster system at z ∼ 0.165 with the STAGES HST ACS survey. We find that the global optical bar fraction in the clusters is ∼ 30% regardless of the method of disk selection. Within a given absolute magnitude bin, the bar fraction increases for galaxies with no significant bulge component. Within each morphological type bin, the bar fraction increases for brighter galaxies. We find no strong trend for the bar fraction with local density within the cluster between the core and virial radius. We discuss the implications of our results for the evolution of bars and disks in dense environments.

KW - Galaxies: clusters: individual: Abell 901/902

KW - Galaxies: evolution

UR - http://www.scopus.com/inward/record.url?scp=84922256443&partnerID=8YFLogxK

M3 - Conference article

SN - 1824-016X

VL - 18

SP - 61

EP - 67

JO - Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society

JF - Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society

T2 - Tumbling, Twisting and Winding Galaxies: Pattern Speeds Along the Hubble Sequence

Y2 - 25 August 2008 through 28 August 2008

ER -

Barred disks in dense environments

Abstract

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