The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

Within the Local Universe galaxies can be studied in great detail star by star, and here we
review the results of quantitative studies in nearby dwarf galaxies. The color-magnitude …

This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral
Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public …

The Lyman decrement associated with the cumulative effect of H i in QSO absorption
systems along the line of sight provides a distinctive feature for identifying galaxies at z≳ 2.5 …

We investigate the relationships between the characteristic oxygen abundance, the radial
abundance gradient, and the macroscopic properties of spiral galaxies by examining the …

Using the output from a grid of 60 Type II supernova models (Woosley\& Weaver 1994) of
varying mass (11$\ltaprx $ M/M\sun $\ltaprx $40) and metallicity (0, 10$^{-4} $, 0.01, 0.1, and …

This paper presents chemical and structural evolutionary models for the Magellanic Clouds
assuming bimodal star formation and gas infall. The models are discussed in relation to the …

H II region abundances - Model oxygen line ratios ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

Abstract Models for chemical evolution of the Galaxy are presented, where the most recent
ideas on stellar nucleosynthesis and supernova (SN) progenitors are taken into account. It is …

In the first paper in this series, we presented a low-density grid of models of high-velocity
photoionizing radiative shocks, including magnetic pressure support in the photoionization …