AGN Feedback in Galaxy Formation Cambridge Contemporary Astrophysics 1st Edition Vincenzo Antonuccio Delogu, Joseph Silk 0521192544 978-0521192545
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Product details:
ISBN 10: 0521192544
ISBN 13: 978-0521192545
Author: Vincenzo Antonuccio Delogu, Joseph Silk
Table of contents:
Part I – AGNs, starbursts and galaxy evolution
1.1 Introduction
1.3 Scaling relations
1.4 Parameter distributions
1.5 The influence of mass
1.6 Star formation inside out
References
2.1 Introduction
2.2 Outline of the model
2.3 Results
2.4 Summary and discussion
References
3.2 Spitzer selection of high-z luminous infrared galaxies
3.3 MAMBO observations and results
3.4 AGN and starburst MIR emission contributions
3.5 Host galaxies
3.6 Average SEDs
3.7 Summary and conclusions
References
4.1 Introduction
4.2 Star formation rates in zCOSMOS galaxies hosting AGN
4.3 Further remarks on color–magnitude diagrams of AGN hosts
4.4 Conclusion: co-evolution of SMBHs and their host galaxies
References
Part II – Co-evolution of black holes and galaxies
5.2 Standard SAMs, their successes and their failures
5.3 Possible solution from joint evolution of QSO and spheroids
5.4 The ABC scenario
References
6.1 Introduction
6.2 Measuring assembly bias in the quasi-linear regime
References
7.2 Hierarchical assembly
7.3 Modelling AGN feedback in galaxies
7.5 Understanding mass errors and cosmic variance
References
Part III – Outflows and radio galaxies
8.1 Why radio-loud AGN?
8.2 The nuclear regions probed by the HI and ionised gas
8.3 Moving to larger scales: jet-induced star formation
8.4 Conclusions
References
9.2 The model: dynamical and spectral evolution
9.3 Comparison with broad-band spectra of GPS galaxies
9.4 Further observational support
9.5 Conclusions and future prospects
References
10.1 Introduction
10.2 Local sample
10.3 Intermittent AGN feedback in galaxy formation
10.4 Summary
References
11.1 Introduction
11.2 Using ultraviolet NALs to reveal QSO feedback
11.3 The line-of-sight distribution of NALs in front of QSOs
11.4 The 3D distribution of NALs around QSOs
11.5 The clustering contribution to the line-of-sight excess
11.6 Radio loud vs. radio quiet
11.7 Conclusions
References
Part IV – Models and numerical simulations: methods and results
12.1 Introduction
12.2 Simulating jet propagation in a two-phase ISM
12.3 Global quenching in elliptical galaxies
12.4 Conclusions
References
13.2 The numerical setup
13.3 Results and discussion
References
14.1 AGN feedback from a radio galaxy perspective
14.4 Jet and disk simulations
14.5 Application to 4C31.04
14.6 Interaction of outflows with individual clouds
14.7 Main points
References
15.1 Introduction
15.2 The simulations
15.3 Temperature profiles
15.4 Metal enrichment of the ICM
15.5 Conclusions
Acknowledgements
References
16.1 Introduction
16.2 Global jet simulations
16.3 Local simulations of multi-phase turbulence
16.4 Discussion and conclusions
References
17.1 Introduction
17.2 The formation of cusps and cores in elliptical galaxies
17.3 Implications for active galactic nuclei in elliptical galaxies
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Tags: Vincenzo Antonuccio Delogu, Joseph Silk, Feedback, Formation