Morphological transformations of galaxies in the A901/02 supercluster from STAGES

Amanda Heiderman; S. Jogee; D. Bacon; M. Balogh; M. Barden; F. D. Barazza; E. F. Bell; A. Boehm; J. A. R. Caldwell; M. E. Gray; B. Haeussler; C. Heymans; K. Jahnke; E. van Kampen; S. Koposov; K. Lane; I. Marinova; D. McIntosh; K. Meisenheimer; C. Y. Peng; H. -W. Rix; S. F. Sanchez; R. Somerville; A. Taylor; L. Wisotzki; C. Wolf; X. Zheng

Morphological transformations of galaxies in the A901/02 supercluster from STAGES

Amanda Heiderman, S. Jogee, D. Bacon, M. Balogh, M. Barden, F. D. Barazza, E. F. Bell, A. Boehm, J. A. R. Caldwell, M. E. Gray, B. Haeussler, C. Heymans, K. Jahnke, E. van Kampen, S. Koposov, K. Lane, I. Marinova, D. McIntosh, K. Meisenheimer, C. Y. PengH. -W. Rix, S. F. Sanchez, R. Somerville, A. Taylor, L. Wisotzki, C. Wolf, X. Zheng

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

We present a study of galaxies in the Abell 901/902 Supercluster at z similar to 0.165, based on HST ACS F606W, COMBO-17, Spitzer 24 mu m, XMM-Newton X-ray, and gravitational lensing maps, as part of the STAGES survey. We characterize galaxies with strong externally-triggered morphological distortions and normal relatively undisturbed galaxies, using visual classification and quantitative CAS parameters. We compare normal and distorted galaxies in terms of their frequency, distribution within the cluster, star formation properties, and relationship to dark matter (DM) or surface mass density, and intra-cluster medium (ICM) density. We revisit the morphology density relation, which postulates a higher fraction of early type galaxies in dense environments, by considering separately galaxies with a low bulge-to-disk (BID) ratio and a low gas content as these two parameters may not he correlated in clusters. We report here on our preliminary analysis.

Original language	English
Title of host publication	NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007
Editors	A Frebel, JR Maund, J Shen, MH Siegel
Place of Publication	SAN FRANCISCO
Publisher	ASTRONOMICAL SOC PACIFIC
Pages	211-214
Number of pages	4
ISBN (Print)	978-1-58381-656-1
Publication status	Published - 2008
Event	Frank N Bash Symposium on New Horizons Astronomy - Austin Duration: 14 Oct 2007 → 16 Oct 2007

Conference

Conference	Frank N Bash Symposium on New Horizons Astronomy
City	Austin
Period	14/10/07 → 16/10/07

Keywords

COMBO-17

Cite this

Heiderman, A., Jogee, S., Bacon, D., Balogh, M., Barden, M., Barazza, F. D., Bell, E. F., Boehm, A., Caldwell, J. A. R., Gray, M. E., Haeussler, B., Heymans, C., Jahnke, K., van Kampen, E., Koposov, S., Lane, K., Marinova, I., McIntosh, D., Meisenheimer, K., ... Zheng, X. (2008). Morphological transformations of galaxies in the A901/02 supercluster from STAGES. In A. Frebel, JR. Maund, J. Shen, & MH. Siegel (Eds.), NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007 (pp. 211-214). ASTRONOMICAL SOC PACIFIC.

@inproceedings{ac0560247f8c4dbfb09bbde85a94ac2d,

title = "Morphological transformations of galaxies in the A901/02 supercluster from STAGES",

abstract = "We present a study of galaxies in the Abell 901/902 Supercluster at z similar to 0.165, based on HST ACS F606W, COMBO-17, Spitzer 24 mu m, XMM-Newton X-ray, and gravitational lensing maps, as part of the STAGES survey. We characterize galaxies with strong externally-triggered morphological distortions and normal relatively undisturbed galaxies, using visual classification and quantitative CAS parameters. We compare normal and distorted galaxies in terms of their frequency, distribution within the cluster, star formation properties, and relationship to dark matter (DM) or surface mass density, and intra-cluster medium (ICM) density. We revisit the morphology density relation, which postulates a higher fraction of early type galaxies in dense environments, by considering separately galaxies with a low bulge-to-disk (BID) ratio and a low gas content as these two parameters may not he correlated in clusters. We report here on our preliminary analysis.",

keywords = "COMBO-17",

author = "Amanda Heiderman and S. Jogee and D. Bacon and M. Balogh and M. Barden and Barazza, {F. D.} and Bell, {E. F.} and A. Boehm and Caldwell, {J. A. R.} and Gray, {M. E.} and B. Haeussler and C. Heymans and K. Jahnke and {van Kampen}, E. and S. Koposov and K. Lane and I. Marinova and D. McIntosh and K. Meisenheimer and Peng, {C. Y.} and Rix, {H. -W.} and Sanchez, {S. F.} and R. Somerville and A. Taylor and L. Wisotzki and C. Wolf and X. Zheng",

year = "2008",

language = "English",

isbn = "978-1-58381-656-1",

pages = "211--214",

editor = "A Frebel and JR Maund and J Shen and MH Siegel",

booktitle = "NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007",

publisher = "ASTRONOMICAL SOC PACIFIC",

note = "Frank N Bash Symposium on New Horizons Astronomy ; Conference date: 14-10-2007 Through 16-10-2007",

}

Heiderman, A, Jogee, S, Bacon, D, Balogh, M, Barden, M, Barazza, FD, Bell, EF, Boehm, A, Caldwell, JAR, Gray, ME, Haeussler, B, Heymans, C, Jahnke, K, van Kampen, E, Koposov, S, Lane, K, Marinova, I, McIntosh, D, Meisenheimer, K, Peng, CY, Rix, H-W, Sanchez, SF, Somerville, R, Taylor, A, Wisotzki, L, Wolf, C & Zheng, X 2008, Morphological transformations of galaxies in the A901/02 supercluster from STAGES. in A Frebel, JR Maund, J Shen & MH Siegel (eds), NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007. ASTRONOMICAL SOC PACIFIC, SAN FRANCISCO, pp. 211-214, Frank N Bash Symposium on New Horizons Astronomy, Austin, 14/10/07.

Morphological transformations of galaxies in the A901/02 supercluster from STAGES. / Heiderman, Amanda; Jogee, S.; Bacon, D. et al.

NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007. ed. / A Frebel; JR Maund; J Shen; MH Siegel. SAN FRANCISCO : ASTRONOMICAL SOC PACIFIC, 2008. p. 211-214.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Morphological transformations of galaxies in the A901/02 supercluster from STAGES

AU - Heiderman, Amanda

AU - Jogee, S.

AU - Bacon, D.

AU - Balogh, M.

AU - Barden, M.

AU - Barazza, F. D.

AU - Bell, E. F.

AU - Boehm, A.

AU - Caldwell, J. A. R.

AU - Gray, M. E.

AU - Haeussler, B.

AU - Heymans, C.

AU - Jahnke, K.

AU - van Kampen, E.

AU - Koposov, S.

AU - Lane, K.

AU - Marinova, I.

AU - McIntosh, D.

AU - Meisenheimer, K.

AU - Peng, C. Y.

AU - Rix, H. -W.

AU - Sanchez, S. F.

AU - Somerville, R.

AU - Taylor, A.

AU - Wisotzki, L.

AU - Wolf, C.

AU - Zheng, X.

PY - 2008

Y1 - 2008

N2 - We present a study of galaxies in the Abell 901/902 Supercluster at z similar to 0.165, based on HST ACS F606W, COMBO-17, Spitzer 24 mu m, XMM-Newton X-ray, and gravitational lensing maps, as part of the STAGES survey. We characterize galaxies with strong externally-triggered morphological distortions and normal relatively undisturbed galaxies, using visual classification and quantitative CAS parameters. We compare normal and distorted galaxies in terms of their frequency, distribution within the cluster, star formation properties, and relationship to dark matter (DM) or surface mass density, and intra-cluster medium (ICM) density. We revisit the morphology density relation, which postulates a higher fraction of early type galaxies in dense environments, by considering separately galaxies with a low bulge-to-disk (BID) ratio and a low gas content as these two parameters may not he correlated in clusters. We report here on our preliminary analysis.

AB - We present a study of galaxies in the Abell 901/902 Supercluster at z similar to 0.165, based on HST ACS F606W, COMBO-17, Spitzer 24 mu m, XMM-Newton X-ray, and gravitational lensing maps, as part of the STAGES survey. We characterize galaxies with strong externally-triggered morphological distortions and normal relatively undisturbed galaxies, using visual classification and quantitative CAS parameters. We compare normal and distorted galaxies in terms of their frequency, distribution within the cluster, star formation properties, and relationship to dark matter (DM) or surface mass density, and intra-cluster medium (ICM) density. We revisit the morphology density relation, which postulates a higher fraction of early type galaxies in dense environments, by considering separately galaxies with a low bulge-to-disk (BID) ratio and a low gas content as these two parameters may not he correlated in clusters. We report here on our preliminary analysis.

KW - COMBO-17

M3 - Conference contribution

SN - 978-1-58381-656-1

SP - 211

EP - 214

BT - NEW HORIZONS IN ASTRONOMY: FRANK N. BASH SYMPOSIUM 2007

A2 - Frebel, A

A2 - Maund, JR

A2 - Shen, J

A2 - Siegel, MH

PB - ASTRONOMICAL SOC PACIFIC

CY - SAN FRANCISCO

T2 - Frank N Bash Symposium on New Horizons Astronomy

Y2 - 14 October 2007 through 16 October 2007

ER -

Morphological transformations of galaxies in the A901/02 supercluster from STAGES

Abstract

Conference

Keywords

Fingerprint

Cite this