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Journal ArticleDOI

MG and Fe absorption features in elliptical galaxies

Guy Worthey, +2 more
- 01 Oct 1992 - 
- Vol. 398, Iss: 1, pp 69-73
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TLDR
In this paper, Fe and Mg indices from two homogenous collections of nuclear elliptical galaxy spectra are compared with model indices. And the average giant elliptical, the [Mg/Fe] ratio exceeds that of the most metal-rich stars in the solar neighborhood by ∼ 0.2-0.3 dex.
Abstract
Fe and Mg indices from two homogenous collections of nuclear elliptical galaxy spectra are compared with model indices. In the average giant elliptical, the [Mg/Fe] ratio exceeds that of the most metal-rich stars in the solar neighborhood by ∼0.2-0.3 dex, with a large spread about this mean. This result implies a variable «enrichment effectiveness» of Type II supernovae (SNs) compared with Type Ia SNs in the evolution of ellipticals, caused perhaps by differences in star formation time scales, the initial mass function, or the amount of Fe versus Mg ejected in galactic winds

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Counting low-mass stars in integrated light

TL;DR: In this paper, a fiducial model was proposed to estimate the initial mass function (IMF) of low-mass stars from integrated flux measurements of old stellar systems, given the numerous variables that can affect the light at the percent level.
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GCD+: a new chemodynamical approach to modelling supernovae and chemical enrichment in elliptical galaxies

TL;DR: In this paper, the authors developed a new galactic chemo-dynamical evolution code, called GCD+, for studies of galaxy formation and evolution, which includes selfgravity, hydrodynamics, radiative cooling, star formation, supernova feedback, and metal enrichment.
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Recovering galaxy stellar population properties from broad-band spectral energy distribution fitting

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Iron as a Tracer in Galaxy Clusters and Groups

TL;DR: In this article, available X-ray data are collected and organized concerning the iron and gas content of galaxy clusters and groups, together with the optical luminosity, mass, and iron abundance of cluster galaxies.
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