2017A&A...602A..84C


Query : 2017A&A...602A..84C

2017A&A...602A..84C - Astronomy and Astrophysics, volume 602A, 84-84 (2017/6-1)

Turbulent gas accretion between supermassive black-holes and star-forming rings in the circumnuclear disk.

CHAMANI W., DORSCHNER S. and SCHLEICHER D.R.G.

Abstract (from CDS):

While supermassive black-holes are known to co-evolve with their host galaxy, the precise nature and origin of this co-evolution is not clear. In this paper we explore the possible connection between star formation and black-hole growth in the circumnuclear disk (CND) to probe this connection in the vicinity close to the black-hole. We adopt here a circumnuclear disk model developed by previous works and explore both the dependence on the star formation recipe as well as the role of the gravitational field, which can be dominated by the central black-hole, the CND itself or the host galaxy. A specific emphasis is put on the turbulence regulated star formation model to explore the impact of a realistic star formation recipe. It is shown that this model helps to introduce realistic fluctuations in the black-hole and star formation rate, without overestimating them. Consistent with previous works, we show that the final black-hole masses are rather insensitive to the masses of the initial seeds, even for seed masses of up to 106M. In addition, we apply our model to the formation of high-redshift quasars, as well as to the nearby system NGC 6951, where a tentative comparison is made in spite of the presence of a bar in the galaxy. We show that our model can reproduce the high black-hole masses of the high-redshift quasars within a sufficiently short time, provided a high mass supply rate from the host galaxy. In addition, it reproduces several of the properties observed in NGC 6951. With respect to the latter system, our analysis suggests that supernovae (SN) feedback may be important in creating the observed fluctuations in the star formation history as a result of negative feedback effects.

Abstract Copyright: © ESO, 2017

Journal keyword(s): quasars: general - galaxies: high-redshift - stars: formation - black hole physics - accretion, accretion disks - turbulence - turbulence

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NGC 613 AGN 01 34 18.235 -29 25 06.56   10.77 12.71 9.50 10.6 ~ 370 3
2 NGC 1097 LIN 02 46 19.059 -30 16 29.68 10.46 9.97 9.48 8.72 9.8 ~ 1221 3
3 QSO J1120+0641 QSO 11 20 01.48 +06 41 24.3           ~ 193 0
4 SDSS J114816.64+525150.3 QSO 11 48 16.647 +52 51 50.31   25.73 25.04     ~ 410 0
5 IC 883 SBG 13 20 35.380 +34 08 21.84   14.8       ~ 378 1
6 Mrk 273 Sy2 13 44 42.164 +55 53 13.53   15.68 14.91     ~ 846 3
7 IC 4553 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 2774 4
8 NGC 6951 Sy2 20 37 14.1181441937 +66 06 20.078027288   11.64 10.65     ~ 507 2

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2021.10.25-23:27:25

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