A New Generation of Parsec-Colibri Stellar Isochrones Including The Tp-Agb Phase
We introduce a new generation of PARSEC-COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB) phase, covering a wide range of initial metallicities (0.0001 < Z i < 0.06). Compared to previous releases, the main novelties and improvements are use of new TP-AGB tracks and related atmosphere models and spectra for M and C-type stars; inclusion of the surface H+He+CNO abundances in the isochrone tables, accounting for the effects of...[Show more]
|Collections||ANU Research Publications|
|Source:||The Astrophysical Journal|
|01_Marigo_A_NEW_GENERATION_of_2017.pdf||5.77 MB||Adobe PDF||Request a copy|
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