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THE FIRST GALAXY FORMATION MODEL WITH THE TPAGB PowerPoint PPT Presentation

THE FIRST GALAXY FORMATION MODEL WITH THE TPAGB - Claudia Maraston, Daniel Thomas (ICG) Julien Devriendt, Joe Silk (University of Oxford) ... Grant 'UniMass' (PI: Claudia Maraston) SIMULATING RED GALAXIES ...

Claudia Maraston, Daniel Thomas (ICG) Julien Devriendt, Joe Silk (University of Oxford) ... Grant 'UniMass' (PI: Claudia Maraston) SIMULATING RED GALAXIES ...

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What can emission lines tell us? lecture 1 Grazyna Stasinska PowerPoint PPT Presentation

What can emission lines tell us? lecture 1 Grazyna Stasinska - What can emission lines tell us? lecture 1 Gra yna Stasi ska

What can emission lines tell us? lecture 1 Gra yna Stasi ska

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THE STELLAR CONTENT OF GALAXIES: RESOLVED STELLAR POPULATIONS I. Theoretical foundations Laura Greggio - OAPd PowerPoint PPT Presentation

THE STELLAR CONTENT OF GALAXIES: RESOLVED STELLAR POPULATIONS I. Theoretical foundations Laura Greggio - OAPd - Review of general properties of stellar tracks, which determine the ... 1.2 Mo. 1 Mo. Flash and After. M tr. RGB tip. RGB base. RGB tip. 10 Ro. 1 Ro. P-EAGB. 100 Ro ...

Review of general properties of stellar tracks, which determine the ... 1.2 Mo. 1 Mo. Flash and After. M tr. RGB tip. RGB base. RGB tip. 10 Ro. 1 Ro. P-EAGB. 100 Ro ...

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Prelim Review PowerPoint PPT Presentation

Prelim Review - Late F stars also show Li depletion due to coupled rotational/wave mixing at ... M , tip of RGB at fixed luminosity (for given z) so acts as standard-ish candle. ...

Late F stars also show Li depletion due to coupled rotational/wave mixing at ... M , tip of RGB at fixed luminosity (for given z) so acts as standard-ish candle. ...

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