Modeling of Dust Spectra of 47 Tucanae with the Help of a Genetic Algorithm

Details Modeling of Dust Spectra of 47 Tucanae with the Help of a Genetic Algorithm Modeling of Dust Spectra of 47 Tucanae with the Help of a Genetic Algorithm

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..313b&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

The mid-infrared spectra of asymptotic giant branch (AGB) stars residing in the globular cluster 47 Tucanae, observed with the Spitzer Space Telescope (Lebzelter et al. 2006), exhibit a variety of significant dust features. In this poster we present model spectrum fits that were generated with an automated fitting procedure first introduced by Dijkstra (2007), which combines the radiative transfer code DUSTY with the genetic algorithm PIKAIA.

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