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THE FIRST GALAXY FORMATION MODEL WITH THE TP-AGB: BASIC REVISION OF THE MASS-LUMINOSITY RELATION

THE FIRST GALAXY FORMATION MODEL WITH THE TP-AGB: BASIC REVISION OF THE MASS-LUMINOSITY RELATION. Obergurgl, December 13th 2009. Chiara Tonini. in collaboration with Claudia Maraston, Daniel Thomas (ICG) Julien Devriendt, Joe Silk (University of Oxford). THE GALAXY FORMATION MODEL.

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264 views • 13 slides

Unravelling the formation and evolutionary histories of the most massive galaxies

Unravelling the formation and evolutionary histories of the most massive galaxies. Ilani Loubser (Univ. of the Western Cape). What is a brightest cluster galaxy?. The central supergiant galaxies in clusters. Embedded in an extensive luminous halo (cD galaxy). Typically : ~10 13 M ?

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325 views • 10 slides

Epoch of Reionization Tomography with the CSO

Epoch of Reionization Tomography with the CSO. Wide-field C+ spectral mapping and correlation with HI Matt Bradford CSO NSF visit: October 12, 2011. Epoch of Reionization. First UV sources turn on and reionize the HI.

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341 views • 8 slides

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Blaizot - PowerPoint PPT Presentation

THE FIRST GALAXY FORMATION MODEL WITH THE TP-AGB: BASIC REVISION OF THE MASS-LUMINOSITY RELATION

Unravelling the formation and evolutionary histories of the most massive galaxies

Epoch of Reionization Tomography with the CSO