The Uncertainties in the Synthetic Indices for Stellar Populations
暂无分享,去创建一个
[1] C. Maraston. Evolutionary synthesis of stellar populations: a modular tool , 1998, astro-ph/9807338.
[2] M. Marconi,et al. Evolutionary and Pulsational Constraints for Super-Metal-rich Stars with Z = 0.04 , 1997 .
[3] D. Ottaviani,et al. Hγ and Hδ Absorption Features in Stars and Stellar Populations , 1997 .
[4] D. Fisher,et al. Line Strength Gradients in Elliptical and Brightest Cluster Galaxies , 1995 .
[5] A. Buzzoni. Evolutionary Population Synthesis in Stellar Systems. II. Early-Type Galaxies , 1995 .
[6] G. Worthey. Comprehensive stellar population models and the disentanglement of age and metallicity effects , 1994 .
[7] David Burstein,et al. Old stellar populations. 5: Absorption feature indices for the complete LICK/IDS sample of stars , 1994 .
[8] L. Mantegazza,et al. Metal enrichment in elliptical galaxies and globular clusters through the study of iron and H-Beta spectral indices , 1994 .
[9] L. Mantegazza,et al. The magnesium Mg2 index as an indicator of metallicity in elliptical galaxies , 1992 .
[10] A. Renzini,et al. Clues on the hot star content and the ultraviolet output of elliptical galaxies , 1990 .
[12] A. Renzini,et al. Spectral Evolution of Galaxies , 1986 .