A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase

We introduce a new generation of PARSEC-COLIBRI stellar isochrones that include a detailed treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) phase, and covering a wide range of initial metallicities (0.0001

Keywords:

• Asymptotic giant branch
• Parsec
• Astrophysics
• Radiative transfer
• Photometry (optics)
• Atmosphere
• Spectral line
• Metallicity
• Physics
• Stars

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