An empirical connection between the ultraviolet color of early-type galaxies and the stellar initial mass function

Dennis F Zaritsky, Armando Gil De Paz, Alexandre Y K Bouquin

Research output: Contribution to journalArticle

5 Citations (Scopus)

Abstract

Using new UV magnitudes for a sample of early-type galaxies (ETGs) with published stellar mass-to-light ratios, Υ*, we find a correlation between UV color and Υ* that is tighter than those previously identified between Υ* and either the central stellar velocity dispersion, metallicity, or alpha enhancement. The sense of the correlation is that galaxies with larger Υ* are bluer in the UV. We conjecture that differences in the lower mass end of the stellar initial mass function (IMF) are related to the nature of the extreme horizontal branch populations that are generally responsible for the UV flux in ETGs. If so, then UV color can be used to identify ETGs with particular IMF properties and to estimate Υ*.

Original languageEnglish (US)
Article numberL1
JournalAstrophysical Journal Letters
Volume780
Issue number1
DOIs
StatePublished - Jan 1 2014

Fingerprint

galaxies
color
mass to light ratios
stellar mass
metallicity
augmentation
estimates

Keywords

  • galaxies: elliptical and lenticular cD
  • galaxies: evolution
  • galaxies: stellar content
  • stars: luminosity function mass function

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

An empirical connection between the ultraviolet color of early-type galaxies and the stellar initial mass function. / Zaritsky, Dennis F; Gil De Paz, Armando; Bouquin, Alexandre Y K.

In: Astrophysical Journal Letters, Vol. 780, No. 1, L1, 01.01.2014.

Research output: Contribution to journalArticle

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