Origin of color gradients in elliptical galaxies

N Tamura, Chiaki Kobayashi, N Arimoto, K Ohta, Tadayuki Kodama

Research output: Contribution to journalArticlepeer-review

58 Citations (Scopus)
61 Downloads (Pure)

Abstract

The origin of color gradients in elliptical galaxies is examined by comparing model gradients with those observed in the Hubble Deep Field. The models are constructed so as to reproduce color gradients in local elliptical galaxies either by a metallicity gradient or by an age gradient. By looking-back a sequence of the color gradient as a function of redshift, the age-metallicity degeneracy is solved. The observed color gradients in elliptical galaxies at z = 0.1 to 1.0 agree excellently with those predicted by the metallicity gradient, while they deviate significantly from those predicted by the age gradient even at z similar to 0.3, and the deviation becomes larger with increasing redshift. This result does not depend on cosmological parameters and parameters for an evolutionary model of an elliptical galaxy within a reasonable range. Thus our results clearly indicate that the origin of color gradients is not age but stellar metallicity.

Original languageEnglish
Pages (from-to)2134-2145
Number of pages12
JournalThe Astronomical Journal
Volume119
Issue number5
DOIs
Publication statusPublished - May 2000

Keywords

  • galaxies : elliptical and lenticular, cD
  • galaxies : evolution
  • galaxies : formation
  • HUBBLE-DEEP-FIELD
  • SURFACE PHOTOMETRY
  • METALLICITY GRADIENTS
  • MAGNITUDE RELATION
  • EVOLUTION
  • SUPERNOVAE
  • DUST
  • FE

Fingerprint

Dive into the research topics of 'Origin of color gradients in elliptical galaxies'. Together they form a unique fingerprint.

Cite this