SIMBAD references

2008ApJ...674...29V - Astrophys. J., 674, 29-50 (2008/February-2)

Evidence of cosmic evolution of the stellar initial mass function.


Abstract (from CDS):

Theoretical arguments and indirect observational evidence suggest that the stellar IMF may evolve with time, such that it is more weighted toward high-mass stars at higher redshift. Here we test this idea by comparing the rate of luminosity evolution of massive early-type galaxies in clusters at 0.02≤z≤0.83 to the rate of their color evolution. A combined fit to the rest-frame U-V color evolution and the previously measured evolution of the M/LB ratio gives x=-0.3+0.4–0.7for the logarithmic slope of the IMF in the region around 1 M, significantly flatter than the present-day value in the Milky Way disk of x=1.3±0.3. The best-fitting luminosity-weighted formation redshift of the stars in massive cluster galaxies is 3.7+2.3–0.8, and a possible interpretation is that the characteristic mass mc had a value of ∼2 Mat z∼4 (compared to mc∼0.1 M today), in qualitative agreement with models in which the characteristic mass is a function of the Jeans mass in molecular clouds. Such a ``bottom-light'' IMF for massive cluster galaxies has significant implications for the interpretation of measurements of galaxy formation and evolution. Applying a simple form of IMF evolution to literature data, we find that the volume-averaged SFR at high redshift may have been overestimated (by a factor of 3-4 at z>4), and the cosmic star formation history may have a fairly well defined peak at z∼1.5. The M/LV ratios of galaxies are less affected than their SFRs, and future data on the stellar mass density at z>3 will provide further constraints on IMF evolution. The formal errors likely underestimate the uncertainties, and confirmation of these results requires a larger sample of clusters and the inclusion of redder rest-frame colors in the analysis.

Abstract Copyright:

Journal keyword(s): Cosmology: Observations - Galaxies: Evolution - Galaxies: Formation

Simbad objects: 22

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