This thesis is a starting point for the TP-AGB phase calibration based on observations of resolved stellar populations in the Small Magellanic Cloud. Using a spatially-resolved SFH, infrared color-magnitude diagrams have been simulated with the population synthesis code TRILEGAL in order to reproduce observed star counts, luminosity functions, color distributions and therefore constrain TP-AGB lifetimes, 3rd DU and mass-loss efficiencies, dust production.
Calibrating the TP-AGR Phase through Resolved Stellar Populations in the Small Magellanic Cloud
Pastorelli, Giada
2015/2016
Abstract
This thesis is a starting point for the TP-AGB phase calibration based on observations of resolved stellar populations in the Small Magellanic Cloud. Using a spatially-resolved SFH, infrared color-magnitude diagrams have been simulated with the population synthesis code TRILEGAL in order to reproduce observed star counts, luminosity functions, color distributions and therefore constrain TP-AGB lifetimes, 3rd DU and mass-loss efficiencies, dust production.File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
pastorelli.pdf
accesso aperto
Dimensione
3.9 MB
Formato
Adobe PDF
|
3.9 MB | Adobe PDF | Visualizza/Apri |
The text of this website © Università degli studi di Padova. Full Text are published under a non-exclusive license. Metadata are under a CC0 License
Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.12608/20243