Multi-phase outflows as probes of AGN accretion history

被引：28

作者：

Nardini, Emanuele ^{[1
]}

Zubovas, Kastytis ^{[2
,3
]}

机构：

[1] Osserv Astrofis Arcetri, INAF, Largo Enrico Fermi 5, I-50125 Florence, Italy

[2] Ctr Phys Sci & Technol, Sauletekio Av 3, LT-10257 Vilnius, Lithuania

[3] Vilnius Univ Observ, Sauletekio Av 3, LT-10257 Vilnius, Lithuania

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2018年 / 478卷 / 02期

基金：

欧盟地平线“2020”;

关键词：

ISM: jets and outflows; galaxies: active; galaxies: evolution; quasars: general; quasars: individual: supermassive black holes; ACTIVE GALACTIC NUCLEI; ULTRALUMINOUS INFRARED GALAXIES; QUASAR PDS 456; BLACK-HOLE; STAR-FORMATION; DRIVEN OUTFLOWS; SCALE OUTFLOWS; COOLING FLOWS; HOST GALAXIES; FEEDBACK;

D O I：

10.1093/mnras/sty1144

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Powerful outflows with a broad range of properties (such as velocity, ionization, radial scale and mass-loss rate) represent a key feature of active galactic nuclei (AGN), even more so since they have been simultaneously revealed also in individual objects. Here we revisit in a simple analytical framework the recent remarkable cases of two ultraluminous infrared quasars, IRAS F11119+3257 and Mrk 231, which allow us to investigate the physical connection between multi-phase AGN outflows across the ladder of distance from the central supermassive black hole (SMBH). We argue that any major deviations from the standard outflow propagation models might encode unique information on the past SMBH accretion history, and briefly discuss how this could help address some controversial aspects of the current picture of AGN feedback.

引用

页码：2274 / 2280

页数：7

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