Constraints on the size evolution of brightest cluster galaxies

Amy E. Nelson, Luc Simard, Dennis F Zaritsky, Julianne J. Dalcanton, Anthony H. Gonzalez

Research output: Contribution to journalArticle

17 Citations (Scopus)

Abstract

We measure the luminosity profiles of 16 brightest cluster galaxies (BCGs) at 0.4 < z < 0.8 using high-resolution F160W NICMOS and F814W WFPC2 Hubble Space Telescope imaging. The heterogeneous sample is drawn from a variety of surveys: seven from clusters in the Einstein Medium Sensitivity Survey, five from the Las Campanas Distant Cluster Survey and its Northern Hemisphere precursor, and the remaining four from traditional optical surveys. We find that the surface brightness profiles of all but three of these BCGs are well described by a standard de Vaucouleurs (r1/4) profile out to at least ∼ 2re and that the biweight-estimated NICMOS effective radius of our high-redshift BCGs (re = 8.3 ± 1.4 kpc for H0 = 80 km s-1 Mpc-1, Ωm = 0.2, ΩΛ = 0.0) is ∼ 2 times smaller than that measured for a local BCG sample. If high-redshift BCGs are in dynamical equilibrium and satisfy the same scaling relations as low-redshift ones, this change in size would correspond to a mass growth of a factor of 2 since z ∼ 0.5. However, the biweight-estimated WFPC2 effective radius of our sample is 18 ± 5.1 kpc, which is fully consistent with the local sample. While we can rule out mass accretion rates higher than a factor of 2 in our sample, the discrepancy between our NICMOS and WFPC2 results, which after various tests we describe appears to be physical, does not yet allow us to place strong constraints on accretion rates below that level.

Original languageEnglish (US)
Pages (from-to)144-154
Number of pages11
JournalAstrophysical Journal
Volume567
Issue number1 I
DOIs
StatePublished - Mar 1 2002

Fingerprint

galaxies
accretion
profiles
Northern Hemisphere
radii
Hubble Space Telescope
brightness
luminosity
scaling
sensitivity
high resolution
rate
test

Keywords

  • Galaxies: clusters: general
  • Galaxies: elliptical and lenticular, cD
  • Galaxies: evolution
  • Galaxies: formation

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Nelson, A. E., Simard, L., Zaritsky, D. F., Dalcanton, J. J., & Gonzalez, A. H. (2002). Constraints on the size evolution of brightest cluster galaxies. Astrophysical Journal, 567(1 I), 144-154. https://doi.org/10.1086/338221

Constraints on the size evolution of brightest cluster galaxies. / Nelson, Amy E.; Simard, Luc; Zaritsky, Dennis F; Dalcanton, Julianne J.; Gonzalez, Anthony H.

In: Astrophysical Journal, Vol. 567, No. 1 I, 01.03.2002, p. 144-154.

Research output: Contribution to journalArticle

Nelson, AE, Simard, L, Zaritsky, DF, Dalcanton, JJ & Gonzalez, AH 2002, 'Constraints on the size evolution of brightest cluster galaxies', Astrophysical Journal, vol. 567, no. 1 I, pp. 144-154. https://doi.org/10.1086/338221
Nelson, Amy E. ; Simard, Luc ; Zaritsky, Dennis F ; Dalcanton, Julianne J. ; Gonzalez, Anthony H. / Constraints on the size evolution of brightest cluster galaxies. In: Astrophysical Journal. 2002 ; Vol. 567, No. 1 I. pp. 144-154.
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