AGN properties in a cosmological evolution scenario

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Standard

AGN properties in a cosmological evolution scenario. / Raimundo, Sandra I.; Fabian, Andrew C.

X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. 2010. s. 497-498 (AIP Conference Proceedings, Bind 1248).

Publikation: Bidrag til bog/antologi/rapport › Konferencebidrag i proceedings › Forskning › fagfællebedømt

Harvard

Raimundo, SI & Fabian, AC 2010, AGN properties in a cosmological evolution scenario. i X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. AIP Conference Proceedings, bind 1248, s. 497-498, International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives, Bologna, Italien, 07/09/2009. https://doi.org/10.1063/1.3475318

APA

Raimundo, S. I., & Fabian, A. C. (2010). AGN properties in a cosmological evolution scenario. I X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference (s. 497-498). AIP Conference Proceedings Bind 1248 https://doi.org/10.1063/1.3475318

Vancouver

Raimundo SI, Fabian AC. AGN properties in a cosmological evolution scenario. I X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. 2010. s. 497-498. (AIP Conference Proceedings, Bind 1248). https://doi.org/10.1063/1.3475318

Author

Raimundo, Sandra I. ; Fabian, Andrew C. / AGN properties in a cosmological evolution scenario. X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives - Proceedings of the International Conference. 2010. s. 497-498 (AIP Conference Proceedings, Bind 1248).

Bibtex

@inproceedings{a5d3007fa25a40b6a77ee0651f3380d0,
title = "AGN properties in a cosmological evolution scenario",
abstract = "To understand how AGN accrete, evolve and affect the surrounding galaxy, it is necessary to investigate how their intrinsic properties change with time. We consider different AGN populations, accounting for the physical properties and obscuration, and trace their redshift evolution. In particular, we investigate the role of Eddington ratio and accretion efficiency in the black hole mass function, and build a scenario where objects with a high spread in Eddington ratios, including low values (10-3-10-2) are consistent with the observed local mass function.",
keywords = "active galaxies, black hole physics",
author = "Raimundo, {Sandra I.} and Fabian, {Andrew C.}",
year = "2010",
doi = "10.1063/1.3475318",
language = "English",
isbn = "9780735407954",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics",
pages = "497--498",
booktitle = "X-ray Astronomy-2009",
note = "International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives ; Conference date: 07-09-2009 Through 11-09-2009",

}

RIS

TY - GEN

T1 - AGN properties in a cosmological evolution scenario

AU - Raimundo, Sandra I.

AU - Fabian, Andrew C.

PY - 2010

Y1 - 2010

N2 - To understand how AGN accrete, evolve and affect the surrounding galaxy, it is necessary to investigate how their intrinsic properties change with time. We consider different AGN populations, accounting for the physical properties and obscuration, and trace their redshift evolution. In particular, we investigate the role of Eddington ratio and accretion efficiency in the black hole mass function, and build a scenario where objects with a high spread in Eddington ratios, including low values (10-3-10-2) are consistent with the observed local mass function.

AB - To understand how AGN accrete, evolve and affect the surrounding galaxy, it is necessary to investigate how their intrinsic properties change with time. We consider different AGN populations, accounting for the physical properties and obscuration, and trace their redshift evolution. In particular, we investigate the role of Eddington ratio and accretion efficiency in the black hole mass function, and build a scenario where objects with a high spread in Eddington ratios, including low values (10-3-10-2) are consistent with the observed local mass function.

KW - active galaxies

KW - black hole physics

UR - http://www.scopus.com/inward/record.url?scp=77955834041&partnerID=8YFLogxK

U2 - 10.1063/1.3475318

DO - 10.1063/1.3475318

M3 - Article in proceedings

AN - SCOPUS:77955834041

SN - 9780735407954

T3 - AIP Conference Proceedings

SP - 497

EP - 498

BT - X-ray Astronomy-2009

T2 - International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives

Y2 - 7 September 2009 through 11 September 2009

ER -

ID: 272400821