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Population Synthesis in the Blue I. Synthesis of the Integrated Spectrum of 47 Tucanae from its Color-Magnitude Diagram | | Ricardo P. Schiavon
; S.M. Faber
; Bruno V. Castilho
; James A. Rose
; | | Date: |
21 Sep 2001 | | Journal: | Astrophys.J. 580 (2002) 850-872 | | Subject: | astro-ph | | Affiliation: | UCO/Lick Observatory, LNA/MCT Brazil, University of North Carolina | | Abstract: | We perform an empirical synthesis of the blue integrated spectrum of the metal-rich globular cluster 47 Tucanae, based directly on the color-magnitude diagram of the cluster coupled to a moderately high-resolution spectral library. Freed from any significant dependence on theory, we are able to perform a fundamental test of the adequacy of the spectral library and its associated stellar parameters. Excellent fits are achieved for almost all absorption-line indices studied, provided the computations are corrected for two limitations of the spectral library, namely, the lack of a representative set of metal-poor giants and the absence of CN-strong stars. The latter effect is corrected by means of spectrum synthesis from model photospheres, considering the abundance pattern of CN-strong and CN-normal stars. We also need to perform a slight correction of the metallicity of the cluster (by --0.05 dex in relation to the standard value [Fe/H]=-0.7) in order to match the metal-line index measurements in the cluster spectrum. After these relatively small adjustments, the overall spectral agreement is good. Good fits are achieved for Hbeta, Hgamma, Mgb, , Ca4227 and Fe4383, and only Hdelta_F is overpredicted. Thus, ages inferred from Hdelta_F are slightly older than the ages based on the other Balmer lines, by ~ 3 Gyrs. The success of this exercise suggests that previous failures to synthesize the spectrum of 47 Tuc must have arisen from inadequacies in the theoretical evolutionary isochrones and/or luminosity functions. Such a possibility is considered in a companion paper. | | Source: | arXiv, astro-ph/0109364 | | Services: | Forum | Review | PDF | Favorites | |
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