The mutual feedback between star fori nation and nuclear activity in large spheroidal galaxies may be a key ingredient to overcome several difficulties plaguing current semi-analytic models for galaxy formation. We discuss some observational implications of the model by Granato et al. for the co-evolution of galaxies and active nuclei at their centers and stress the potential of the forthcoming surveys of the Sunyaev-Zeldovich effect on arcminute scales, down to muK levels, to investigate the early galaxy-formation phases, difficult to access by other means.

Observational tests of the galaxy formation process

Danese, Luigi
2004-01-01

Abstract

The mutual feedback between star fori nation and nuclear activity in large spheroidal galaxies may be a key ingredient to overcome several difficulties plaguing current semi-analytic models for galaxy formation. We discuss some observational implications of the model by Granato et al. for the co-evolution of galaxies and active nuclei at their centers and stress the potential of the forthcoming surveys of the Sunyaev-Zeldovich effect on arcminute scales, down to muK levels, to investigate the early galaxy-formation phases, difficult to access by other means.
2004
294
1-2
3
8
De Zotti, G; Granato, Gl; Silva, L; Danese, Luigi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/13678
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