Population Synthesis in the Blue IV: Accurate Model Predictions for Lick Indices and UBV Colors in Single Stellar Populations
arXiv:astro-ph/0611464 · doi:10.1086/511753
Abstract
[Abridged] We present new model predictions for 16 Lick absorption line indices from Hdelta through Fe5335, and UBV colors for single stellar populations (SPs) with ages ranging between 1 and 15 Gyr, [Fe/H] ranging from -1.3 to +0.3, and variable abundance ratios. We develop a method to estimate mean ages and abundances of Fe, C, N, Mg, and Ca that explores the sensitivity of the various indices to those parameters. When applied to high-S/N Galactic cluster data, the models match the clusters' elemental abundances and ages with high precision. Analyzing stacked SDSS spectra of early-type galaxies brighter than Lstar, we find mean luminosity-weighted ages of the order of ~ 8 Gyr and iron abundances slightly below solar. Abundance ratios, [X/Fe], are higher than solar, and correlate positively with galaxy luminosity. Nitrogen is the element whose abundance correlates the most strongly with luminosity, which seems to indicate secondary enrichment. This result may impose a lower limit of 50-200 Myr to the time-scale of star formation in early-type galaxies. Unlike in the case of clusters, in galaxies bluer Balmer lines yield younger ages than Hbeta. This age discrepancy is stronger for lower luminosity galaxies. We examine four scenarios to explain this trend. The most likely is the presence of small amounts of a young/intermediate-age SP component. Two-component models provide a better match to the data when the mass fraction of the young component is a few %. This result implies that star formation has been extended in early-type galaxies, and more so in less massive galaxies, lending support to the ``downsizing'' scenario. It also implies that SP synthesis models are capable of constraining not only the mean ages of SPs in galaxies, but also their age spread.
arXiv commentTo appear in the Astrophysical Journal Supplement Series. 55 Pages, using emulateapj5.sty. Full version, containing all (enlarged) figures can be found at http://www.astro.virginia.edu/~rps7v/Models/ms.pdf . A number of useful tables in the Appendix can be obtained in advance of publication by request to the author
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- Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
- Multiple populations within globular clusters in Early-type galaxies Exploring their effect on stellar initial mass function estimates
- The Galaxy Population of Abell 1367: The Stellar Mass-Metallicity Relation
- The Sami Galaxy Survey: stellar populations of passive spiral galaxies in different environment
- An empirical calibration of Lick indices using Milky Way Globular Clusters
- Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
- Galaxy evolution from "dis"integrated light
- The origin of the nuclear star-forming ring in NGC 3182
- The stellar populations in the low luminosity, early-type galaxy NGC59
- Counting stars from the integrated spectra of galaxies
- Hidden Figures of Globular Clusters: Integrated Stellar Populations Impacted by Hot Subdwarfs
- The star formation timescale of elliptical galaxies -- Fitting [Mg/Fe] and total metallicity simultaneously
- Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
- A Comparison of Full Spectral Fitting Codes for Measuring the Stellar Initial Mass Function and Other Stellar Population Properties in Elliptical Galaxies
- Photometric and Spectroscopic Study of Abell 0671
- Fundamental parameters of some B-type stars using NOAO Indo-U.S. Library
- Connection between dynamically derived IMF normalisation and stellar populations
- Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
- Spatially Resolved Kinematics of Post-starburst Galaxies
- Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
- SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
- UCDs in the Coma Cluster
- Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
- SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
- Challenges in Stellar Population Studies