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000002899 0247_ $$2DOI$$a10.1017/S1743921308028743
000002899 037__ $$aASTROimport-1056
000002899 100__ $$aMarigo, P.
000002899 245__ $$aThermally-pulsing asymptotic giant branch stars in the Magellanic Clouds
000002899 260__ $$c2009
000002899 520__ $$aWe present the latest results of a theoretical project aimed at investigating the properties of thermally-pulsing asymptotic giant branch (TP-AGB) stars in different host systems. For this purpose, we have recently calculated calibrated synthetic TP-AGB tracks — covering a wide range of metallicities (0.0001 = Z = 0.03) up to the complete ejection of the envelope by stellar winds (Marigo  Girardi 2007) — and used them to generate new sets of stellar isochrones (Marigo et al. 2008). The latter are converted to about 25 different photometric systems, including the mid-infrared filters of Spitzer and AKARI as the effect of circumstellar dust from AGB stars is taken into account. First comparisons with AGB data in the MC field and stellar clusters are discussed. 
000002899 700__ $$a Girardi, L.
000002899 700__ $$a Bressan, A.
000002899 700__ $$a Groenewegen, M. A. T.
000002899 700__ $$a Aringer, B.
000002899 700__ $$a Silva, L.
000002899 700__ $$a Granato, G. L.
000002899 773__ $$c385-390$$pThe Magellanic System: Stars, Gas, and Galaxies$$v256$$y2009
000002899 85642 $$ahttp://esoads.eso.org/abs/2009IAUS..256..385M
000002899 905__ $$apublished in
000002899 980__ $$aNONREF