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AGN Feedback in Galaxy Formation [Kietas viršelis]

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  • Formatas: Hardback, 218 pages, aukštis x plotis x storis: 254x180x15 mm, weight: 590 g, 18 Halftones, black and white; 66 Line drawings, black and white
  • Serija: Cambridge Contemporary Astrophysics
  • Išleidimo metai: 28-Oct-2010
  • Leidėjas: Cambridge University Press
  • ISBN-10: 0521192544
  • ISBN-13: 9780521192545
Kitos knygos pagal šią temą:
AGN Feedback in Galaxy FormationDidesnis paveikslėlis
  • Formatas: Hardback, 218 pages, aukštis x plotis x storis: 254x180x15 mm, weight: 590 g, 18 Halftones, black and white; 66 Line drawings, black and white
  • Serija: Cambridge Contemporary Astrophysics
  • Išleidimo metai: 28-Oct-2010
  • Leidėjas: Cambridge University Press
  • ISBN-10: 0521192544
  • ISBN-13: 9780521192545
Kitos knygos pagal šią temą:
Pastovi nuoroda: https://www.kriso.lt/db/9780521192545.html
Raktažodžiai:
"During the past decade, convincing evidence has been accumulated concerning the effect of active galactic nuclei (AGN) activity on the internal and external environment of their host galaxies. Featuring contributions from well-respected researchers in the field, and bringing together work by specialists in both galaxy formation and AGN, this volume addresses a number of key questions about AGN feedback in the context of galaxy formation. The topics covered include downsizing and star-formation time scales in massive elliptical galaxies, the connection between the epochs of supermassive black hole growth and galaxy formation and the question of whether AGN and star formation coexist. Authors also discuss key challenging computational problems, including jet-interstellar/intergalactic medium interactions, and both jet- and merging-induced star formation. Suitable for researchers and graduate students in astrophysics, this volume reflects the engaging and lively discussions taking place in this emerging field of research"--Provided by publisher.

Provided by publisher.

Recenzijos

' a well-rounded summary of the recent status of this fast-moving research field, as well as a discussion of some of the most important outstanding problems.' The Observatory

Daugiau informacijos

Suitable for researchers and graduate students in astrophysics, this volume discusses AGN feedback in the context of galaxy formation.
List of contributors
x
Preface xiii
The organising committees xv
Part I AGNs, starbursts and galaxy evolution
1(38)
1 The effects of mass and star-formation timescale on galaxy evolution
3(8)
C.D. Harrison
M. Colless
1.1 Introduction
3(1)
1.2 Estimating the stellar population parameters
4(1)
1.3 Scaling relations
4(2)
1.4 Parameter distributions
6(1)
1.5 The influence of mass
7(1)
1.6 Star formation inside out
8(2)
1.7 Summary
10(1)
References
10(1)
2 Suppressing cluster cooling flows by multiple AGN activity
11(10)
A. Nusser
2.1 Introduction
11(1)
2.2 Outline of the model
12(5)
2.3 Results
17(1)
2.4 Summary and discussion
18(3)
References
20(1)
3 Starburst and AGN activity in Spitzer-selected sources at high-z
21(8)
M. Polletta
A. Omont
C. Lonsdale
D. Shupe
3.1 Introduction
21(1)
3.2 Spitzer selection of high-z luminous infrared galaxies
21(2)
3.3 MAMBO observations and results
23(1)
3.4 AGN and starburst MIR emission contributions
24(1)
3.5 Host galaxies
25(1)
3.6 Average SEDs
26(1)
3.7 Summary and conclusions
27(2)
References
28(1)
4 Star formation in galaxies hosting active galactic nuclei up to z ~ 1
29(10)
J. D. Silverman
4.1 Introduction
29(3)
4.2 Star formation rates in zCOSMOS galaxies hosting AGN
32(1)
4.3 Further remarks on color-magnitude diagrams of AGN hosts
33(2)
4.4 Conclusion: co-evolution of SMBHs and their host galaxies
35(4)
References
36(3)
Part II Co-evolution of black holes and galaxies
39(22)
5 The symbiosis between galaxies and SMBHs
41(6)
G. L. Granato
M. Cook
A. Lapi
L. Silva
5.1 Introduction
41(1)
5.2 Standard SAMs, their successes and their failures
41(2)
5.3 Possible solution from joint evolution of QSO and spheroids
43(1)
5.4 The ABC scenario
44(3)
References
45(2)
6 On the origin of halo assembly bias
47(5)
A. Keselman
6.1 Introduction
47(2)
6.2 Measuring assembly bias in the quasi-linear regime
49(1)
6.3 Conclusions
50(2)
References
50(2)
7 AGN, downsizing and galaxy bimodality
52(9)
M. J. Stringer
A. J. Benson
K. Bundy
R. S. Ellis
7.1 Introduction
52(1)
7.2 Hierarchical assembly
52(2)
7.3 Modelling AGN feedback in galaxies
54(2)
7.4 Colour bimodality
56(1)
7.5 Understanding mass errors and cosmic variance
56(5)
Acknowledgements
59(1)
References
59(2)
Part III Outflows and radio galaxies
61(48)
8 Interaction and gas outflows in radio-loud AGN: disruptive and constructive effects of radio jets
63(12)
R. Morganti
8.1 Why radio-loud AGN?
63(2)
8.2 The nuclear regions probed by the HI and ionised gas
65(4)
8.3 Moving to larger scales: jet-induced star formation
69(3)
8.4 Conclusions
72(3)
Acknowledgements
73(1)
References
73(2)
9 Young radio sources: evolution and broad-band emission
75(7)
L. Ostorero
R. Moderski
L. Stawarz
M. Begelman
A. Diaferio
I. Kowalska
J. Kataoka
S. J. Wagner
9.1 Introduction
75(1)
9.2 The model: dynamical and spectral evolution
75(2)
9.3 Comparison with broad-band spectra of GPS galaxies
77(1)
9.4 Further observational support
78(2)
9.5 Conclusions and future prospects
80(2)
Acknowledgements
81(1)
References
81(1)
10 The duty cycle of radio galaxies and AGN feedback
82(16)
S. Shabala
10.1 Introduction
82(1)
10.2 Local sample
83(5)
10.3 Intermittent AGN feedback in galaxy formation
88(7)
10.4 Summary
95(3)
Acknowledgements
96(1)
References
96(2)
11 Environment or outflows? New insight into the origin of narrow associated QSO absorbers
98(11)
V. Wild
11.1 Introduction
98(1)
11.2 Using ultraviolet NALs to reveal QSO feedback
99(2)
11.3 The line-of-sight distribution of NALs in front of QSOs
101(1)
11.4 The 3D distribution of NALs around QSOs
102(2)
11.5 The clustering contribution to the line-of-sight excess
104(1)
11.6 Radio loud vs. radio quiet
105(1)
11.7 Conclusions
106(3)
Acknowledgements
107(1)
References
107(2)
Part IV Models and numerical simulations: methods and results
109(91)
12 Physical models of AGN feedback
111(46)
V. Antonuccio-Delogu
J. Silk
C. Tortora
S. Kaviraj
N. Napolitano
A. D. Romeo
12.1 Introduction
111(1)
12.2 Simulating jet propagation in a two-phase ISM
112(17)
12.3 Global quenching in elliptical galaxies
129(22)
12.4 Conclusions
151(6)
References
154(3)
13 Large-scale expansion of AGN outflows in a cosmological volume
157(8)
P. Barai
13.1 Introduction
157(1)
13.2 The numerical setup
157(3)
13.3 Results and discussion
160(5)
References
163(2)
14 Relativistic jets and the inhomogeneous interstellar medium
165(10)
G. V. Bicknell
J. L. Cooper
R. S. Sutherland
14.1 AGN feedback from a radio galaxy perspective
165(1)
14.2 Simulation code
166(1)
14.3 Isotropisation of jet momentum
166(1)
14.4 Jet and disk simulations
166(3)
14.5 Application to 4C31.04
169(2)
14.6 Interaction of outflows with individual clouds
171(1)
14.7 Main points
172(3)
References
174(1)
15 AGN feedback effect on intracluster medium properties from galaxy cluster hydrodynamical simulations
175(8)
D. Fabjan
S. Borgani
L. Tornatore
A. Saro
K. Dolag
15.1 Introduction
175(1)
15.2 The simulations
176(1)
15.3 Temperature profiles
177(1)
15.4 Metal enrichment of the ICM
178(2)
15.5 Conclusions
180(3)
Acknowledgements
181(1)
References
182(1)
16 Physics and fate of jet-related emission line regions
183(11)
M. G. H. Krause
V. Gaibler
16.1 Introduction
183(2)
16.2 Global jet simulations
185(2)
16.3 Local simulations of multi-phase turbulence
187(3)
16.4 Discussion and conclusions
190(4)
References
192(2)
17 Cusp-core dichotomy of elliptical galaxies: the role of thermal evaporation
194(6)
C. Nipoti
17.1 Introduction
194(1)
17.2 The formation of cusps and cores in elliptical galaxies
195(2)
17.3 Implications for active galactic nuclei in elliptical galaxies
197(1)
17.4 Conclusions
198(2)
Acknowledgements
198(1)
References
198(2)
Index 200
Vincenzo Antonuccio-Delogu is a research astronomer at the Italian National Institute for Astrophysics, Osservatorio Astrofisico di Catania, Italy. His research focuses on dynamics and substructure in clusters of galaxies, parallel N-body simulation codes and galaxy formation and evolution. Joseph Silk is Savilian Professor of Astronomy at the University of Oxford, and Director of the Beecroft Institute of Particle Astrophysics and Cosmology (BIPAC). His research interests include theoretical cosmology, dark matter, galaxy formation and the cosmic microwave background.