NDLI: Models of AGN feedback

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Models of AGN feedback

Content Provider	Scilit
Author	Combes, Françcoise
Copyright Year	2014
Description	The physical processes responsible of sweeping up the surrounding gas in the host galaxy of an AGN, and able in some circumstances to expel it from the galaxy, are not yet well known. The various mechanisms are briefly reviewed: quasar or radio modes, either momentum-conserving outflows, energy-conserving outflows, or intermediate. They are confronted to observations, to know whether they can explain the M-sigma relation, quench the star formation or whether they can also provide some positive feedback and how the black hole accretion history is related to that of star formation.
Related Links	http://arxiv.org/abs/1408.1591 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/34C98B26205E3DB6F30230651043B0A3/S1743921314009636a.pdf/div-class-title-models-of-agn-feedback-div.pdf
Ending Page	189
Page Count	8
Starting Page	182
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921314009636
Journal	Proceedings of the International Astronomical Union
Issue Number	S309
Volume Number	10
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2014-07-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Elliptical and Lenticular Galaxies
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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