Luminosity Evolution of Early-type Galaxies to z=0.83: Constraints on Formation Epoch and Omega

Details Luminosity Evolution of Early-type Galaxies to z=0.83: Constraints on Formation Epoch and Omega Luminosity Evolution of Early-type Galaxies to z=0.83: Constraints on Formation Epoch and Omega

1998-07-23

arxiv.org/abs/astro-ph/9807242v1

Astrophys.J.504:L17,1998

Astronomy and Astrophysics

Astrophysics

To be published in ApJ Letters, Volume 504, September 1, 1998. 5 pages, 4 figures

Scientific paper

10.1086/311567

We present deep spectroscopy with the Keck telescope of eight galaxies in the luminous X-ray cluster MS1054-03 at z=0.83. The data are combined with imaging observations from the Hubble Space Telescope (HST). The spectroscopic data are used to measure the internal kinematics of the galaxies, and the HST data to measure their structural parameters. Six galaxies have early-type spectra, and two have "E+A" spectra. The galaxies with early-type spectra define a tight Fundamental Plane (FP) relation. The evolution of the mass-to-light ratio is derived from the FP. The M/L ratio evolves as \Delta log M/L_B \propto -0.40 z (Omega_m=0.3, Omega_Lambda=0). The observed evolution of the M/L ratio provides a combined constraint on the formation redshift of the stars, the IMF, and cosmological parameters. For a Salpeter IMF (x=2.35) we find that z_form>2.8 and Omega_m<0.86 with 95% confidence. The constraint on the formation redshift is weaker if Omega_Lambda>0: z_form>1.7 if Omega_m=0.3 and Omega_Lambda=0.7. At present the limiting factor in constraining z_form and Omega from the observed luminosity evolution of early-type galaxies is the poor understanding of the IMF. We find that if Omega_m=1 the IMF must be significantly steeper than the Salpeter IMF (x>2.6).

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