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Hubble Space Telescope survey of the Perseus cluster, III: the effect of local environment on dwarf galaxies

Samantha J Penny, Christopher J Conselice, Sven De Rijcke UGent, Enrico V Held, John S Gallagher and Robert W O'Connell (2011) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 410(2). p.1076-1088
abstract
We present the results of a Hubble Space Telescope (HST) study of dwarf galaxies in the outer regions of the nearby rich Perseus cluster, down to M-V = -12, and compare these with the dwarf population in the cluster core from our previous HST imaging. In this paper, we examine how properties such as the colour-magnitude relation, structure and morphology are affected by environment for the lowest mass galaxies. Dwarf galaxies are excellent tracers of the effects of environment due to their low masses, allowing us to derive their environmentally based evolution, which is more subtle in more massive galaxies. We identify 11 dwarf elliptical (dE) and dwarf spheroidal (dSph) galaxies in the outer regions of Perseus, all of which are previously unstudied. We measure the (V - I)(0) colours of our newly discovered dEs, and find that these dwarfs lie on the same red sequence as those in the cluster core. The morphologies of these dwarfs are examined by quantifying their light distributions using concentration, asymmetry and clumpiness (CAS) parameters, and we find that dEs in the cluster outskirts are on average more disturbed than those in the core, with << A >> = 0.13 +/- 0.09 and << S >> = 0.18 +/- 0.08, compared to << A >> = 0.02 +/- 0.04, << S >> = 0.01 +/- 0.07 for those in the core. Based on these results, we infer that these objects are 'transition dwarfs', likely in the process of transforming from late-type to early-type galaxies as they infall into the cluster, with their colours transforming before their structures. When we compare the number counts for both the core and outer regions of the cluster, we find that below M-V = -12, the counts in the outer regions of the cluster exceed those in the core. This is evidence that in the very dense region of the cluster, dwarfs are unable to survive unless they are sufficiently massive to prevent their disruption by the cluster potential and interactions with other galaxies.
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
keyword
galaxies: clusters: individual: Perseus cluster, galaxies: clusters: general, galaxies: dwarf, LOW-MASS GALAXIES, VIRGO CLUSTER, ELLIPTIC GALAXIES, STELLAR POPULATIONS, SPHEROIDAL GALAXIES, LUMINOSITY FUNCTION, EVOLUTION, ORIGIN, DISTRIBUTIONS, KINEMATICS
journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Mon. Not. Roy. Astron. Soc.
volume
410
issue
2
pages
1076 - 1088
Web of Science type
Article
Web of Science id
000285766000028
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
4.9 (2011)
JCR rank
9/56 (2011)
JCR quartile
1 (2011)
ISSN
0035-8711
DOI
10.1111/j.1365-2966.2010.17506.x
language
English
UGent publication?
yes
classification
A1
copyright statement
I have transferred the copyright for this publication to the publisher
id
1843116
handle
http://hdl.handle.net/1854/LU-1843116
date created
2011-06-28 10:43:10
date last changed
2016-12-19 15:39:53
@article{1843116,
  abstract     = {We present the results of a Hubble Space Telescope (HST) study of dwarf galaxies in the outer regions of the nearby rich Perseus cluster, down to M-V = -12, and compare these with the dwarf population in the cluster core from our previous HST imaging. In this paper, we examine how properties such as the colour-magnitude relation, structure and morphology are affected by environment for the lowest mass galaxies. Dwarf galaxies are excellent tracers of the effects of environment due to their low masses, allowing us to derive their environmentally based evolution, which is more subtle in more massive galaxies. We identify 11 dwarf elliptical (dE) and dwarf spheroidal (dSph) galaxies in the outer regions of Perseus, all of which are previously unstudied. We measure the (V - I)(0) colours of our newly discovered dEs, and find that these dwarfs lie on the same red sequence as those in the cluster core. The morphologies of these dwarfs are examined by quantifying their light distributions using concentration, asymmetry and clumpiness (CAS) parameters, and we find that dEs in the cluster outskirts are on average more disturbed than those in the core, with {\textlangle}{\textlangle} A {\textrangle}{\textrangle} = 0.13 +/- 0.09 and {\textlangle}{\textlangle} S {\textrangle}{\textrangle} = 0.18 +/- 0.08, compared to {\textlangle}{\textlangle} A {\textrangle}{\textrangle} = 0.02 +/- 0.04, {\textlangle}{\textlangle} S {\textrangle}{\textrangle} = 0.01 +/- 0.07 for those in the core. Based on these results, we infer that these objects are 'transition dwarfs', likely in the process of transforming from late-type to early-type galaxies as they infall into the cluster, with their colours transforming before their structures. When we compare the number counts for both the core and outer regions of the cluster, we find that below M-V = -12, the counts in the outer regions of the cluster exceed those in the core. This is evidence that in the very dense region of the cluster, dwarfs are unable to survive unless they are sufficiently massive to prevent their disruption by the cluster potential and interactions with other galaxies.},
  author       = {Penny, Samantha J and Conselice, Christopher J and De Rijcke, Sven and Held, Enrico V and Gallagher, John S and O'Connell, Robert W},
  issn         = {0035-8711},
  journal      = {MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY},
  keyword      = {galaxies: clusters: individual: Perseus cluster,galaxies: clusters: general,galaxies: dwarf,LOW-MASS GALAXIES,VIRGO CLUSTER,ELLIPTIC GALAXIES,STELLAR POPULATIONS,SPHEROIDAL GALAXIES,LUMINOSITY FUNCTION,EVOLUTION,ORIGIN,DISTRIBUTIONS,KINEMATICS},
  language     = {eng},
  number       = {2},
  pages        = {1076--1088},
  title        = {Hubble Space Telescope survey of the Perseus cluster, III: the effect of local environment on dwarf galaxies},
  url          = {http://dx.doi.org/10.1111/j.1365-2966.2010.17506.x},
  volume       = {410},
  year         = {2011},
}

Chicago
Penny, Samantha J, Christopher J Conselice, Sven De Rijcke, Enrico V Held, John S Gallagher, and Robert W O’Connell. 2011. “Hubble Space Telescope Survey of the Perseus Cluster, III: The Effect of Local Environment on Dwarf Galaxies.” Monthly Notices of the Royal Astronomical Society 410 (2): 1076–1088.
APA
Penny, S. J., Conselice, C. J., De Rijcke, S., Held, E. V., Gallagher, J. S., & O’Connell, R. W. (2011). Hubble Space Telescope survey of the Perseus cluster, III: the effect of local environment on dwarf galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 410(2), 1076–1088.
Vancouver
1.
Penny SJ, Conselice CJ, De Rijcke S, Held EV, Gallagher JS, O’Connell RW. Hubble Space Telescope survey of the Perseus cluster, III: the effect of local environment on dwarf galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2011;410(2):1076–88.
MLA
Penny, Samantha J, Christopher J Conselice, Sven De Rijcke, et al. “Hubble Space Telescope Survey of the Perseus Cluster, III: The Effect of Local Environment on Dwarf Galaxies.” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 410.2 (2011): 1076–1088. Print.