Cluster galaxy evolution from a new sample of galaxy clusters at 0.3 < z < 0.9

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

Research output: Contribution to journalArticle

22 Citations (Scopus)

Abstract

We analyze photometry and spectroscopy of a sample of 63 clusters at 0.3 ≤ z ≤ 0.9 drawn from the Las Campanas Distant Cluster Survey to empirically constrain models of cluster galaxy evolution. Specifically, (1) by combining I-band photometry of 44 of our clusters with that of 19 clusters from the literature, we parameterize the redshift dependence of M*I in the observed frame as M*I = (-21.74 ± 0.12) - (0.88 + 0.24)z - 5 log h (rms deviation = 0.34) for 0.3 ≤ z ≤ 0.9 (Ω0 = 02, ΩΛ = 0); (2) by combining 30 of our clusters and 14 clusters from the literature with V and I data, we parameterize the redshift dependence of the V-I color of the E/S0 red sequence in the observed frames as V-I = (-0.24 ± 0.28) + (7.42 ± 1.03)z - (4.61 ± 0.91)z2 (rms deviation = 0.16) for 0.3 ≤ z ≤ 0.9; and (3) by combining 13 of our clusters with 15 clusters from the literature with I and K′ data, we parameterize the redshift dependence of the I-K′ color of the E/S0 red sequence in the observed frames as I-K′ = (0.66 ± 0.65) + (9.50 ± 3.72)z - (14.72 ± 7.01)z2 + (8.72 ± 4.29)z3 (rms deviation = 0.18) for 0.3 ≤ z ≤ 0.9. Using the peak surface brightness of the cluster detection, Σ, as a proxy for cluster mass, we find no correlation between Σ and M*I or the location of the red envelope in V-I. We suggest that these observations can be explained with a model in which luminous early-type galaxies (or more precisely, the progenitors of current-day luminous early-type galaxies) form the bulk of their stellar populations at high redshifts (≳5) and in which many of these galaxies, if not all, accrete mass either in the form of evolved stellar populations or gas that causes only a short-term episode of star formation at lower redshifts (1.5 < z < 2). Our data are too crude to reach conclusions regarding the evolutionary state of any particular cluster or to investigate whether the morphological evolution of galaxies matches the simple scenario that we discuss, but the statistical nature of this study suggests that the observed evolutionary trends are universal in massive clusters.

Original languageEnglish (US)
Pages (from-to)629-652
Number of pages24
JournalAstrophysical Journal
Volume563
Issue number2 PART 1
DOIs
StatePublished - Dec 20 2001

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galaxies
spectroscopy
gas
deviation
photometry
color
star formation
brightness
envelopes
trends
detection
trend
causes
gases

Keywords

  • Galaxies: clusters: general
  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: photometry
  • Surveys

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Cluster galaxy evolution from a new sample of galaxy clusters at 0.3 < z < 0.9. / Nelson, Amy E.; Gonzalez, Anthony H.; Zaritsky, Dennis F; Dalcanton, Julianne J.

In: Astrophysical Journal, Vol. 563, No. 2 PART 1, 20.12.2001, p. 629-652.

Research output: Contribution to journalArticle

Nelson, Amy E. ; Gonzalez, Anthony H. ; Zaritsky, Dennis F ; Dalcanton, Julianne J. / Cluster galaxy evolution from a new sample of galaxy clusters at 0.3 < z < 0.9. In: Astrophysical Journal. 2001 ; Vol. 563, No. 2 PART 1. pp. 629-652.
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