2007MNRAS.374L..10P


Query : 2007MNRAS.374L..10P

2007MNRAS.374L..10P - Mon. Not. R. Astron. Soc., 374, L10-L14 (2007/January-1)

Kinetically dominated FRII radio sources.

PUNSLY B.

Abstract (from CDS):

The existence of Fanaroff-Riley class II objects that are kinetically dominated, the jet kinetic luminosity, Q, is larger than the total thermal luminosity (infrared to X-ray) of the accretion flow, Lbol, is of profound theoretical interest. Such objects are not expected in most theoretical models of the central engine of radio-loud active galactic nuclei. Thus, establishing such a class of objects is an important diagnostic for filtering through the myriad of theoretical possibilities. This Letter attempts to establish a class of quasars that have existed in a state of kinetic dominance, R(t) ≡ Q(t)/Lbol(t) > 1, at some epoch, t. It is argued that the 10 quasars in this article with a long-term time-average, that exceeds LEddare likely to have satisfied the condition R(t) > 1 either presently or in the past based on the rarity of Lbol> LEddquasars. Finally, the existence of these sources is discussed in the context of the theory of the central engine.

Abstract Copyright: 2006 The Author. Journal compilation © 2006 RAS

Journal keyword(s): accretion, accretion discs - black hole physics - galaxies: active - galaxies: jets - quasars: general

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 2C 26 BLL 00 20 25.2231670656 +15 40 54.774271884   17.92 17.62     ~ 342 1
2 2C 44 QSO 00 36 06.4449136608 +18 37 59.099054268   20 20     ~ 120 1
3 3C 82 QSO 03 14 43.6 +43 14 05     21.0     ~ 51 2
4 4C 25.21 QSO 07 33 08.7783505488 +25 36 25.007342256   19.60 19.26     ~ 76 1
5 3C 190 QSO 08 01 33.5525166480 +14 14 42.813906612   21.07 20.26 18.972   ~ 242 2
6 ICRF J090933.4+425346 Sy2 09 09 33.49714902 +42 53 46.4821036   19.98 19.42 18.220   ~ 503 0
7 QSO B1017-426 QSO 10 20 03.9200896584 -42 51 30.043737900     18.9     ~ 48 1
8 7C 1218+3359 QSO 12 20 33.8756544048 +33 43 12.026168040   18.80 18.61     ~ 266 1
9 3C 455.0 Sy2 22 55 03.8 +13 13 34   19.535 19.590 19.190   ~ 193 2
10 4C 04.81 QSO 23 40 57.9777278016 +04 31 15.569002452   20.0 19.5     ~ 82 1

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