2012MNRAS.422.1453N

Query : 2012MNRAS.422.1453N

2012MNRAS.422.1453N - Mon. Not. R. Astron. Soc., 422, 1453-1459 (2012/May-2)

The radio core of the ultraluminous infrared galaxy F00183-7111: watching the birth of a quasar.

NORRIS R.P., LENC E., ROY A.L. and SPOON H.

Abstract (from CDS):

F00183-7111 is one of the most extreme ultraluminous infrared galaxies known, with a bolometric luminosity of 9 {x} 1012 L☉. Here we present a very long baseline interferometry (VLBI)_ image which shows a compact core-jet active galactic nucleus (AGN) in its core, with a radio luminosity (L_2.3 GHz_= 6 {x} 1025 W/Hz) typical of powerful radio galaxies. Although already radio loud, the quasar jets are only 1.7 kpc long, boring through the dense gas and starburst activity that confine them. This source therefore appears to be powered by a combination of a compact radio-loud AGN surrounded by vigorous starburst activity.

Abstract Copyright: 2012 CSIRO Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): galaxies: active - galaxies: evolution - galaxies: jets - radio continuum: galaxies

CDS comments: Object 0313-192 = [LO95] 0313-192

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 IRAS 00182-7112 Sy2 00 20 34.72104 -70 55 26.2488     20.6     ~ 143 0
2 NGC 612 Sy2 01 33 57.751 -36 29 35.80   13.90 13.15 12.33   ~ 252 0
3 LEDA 97372 Sy2 03 15 52.11290 -19 06 44.2368   17.48       ~ 62 1
4 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
5 NGC 3256 Sy2 10 27 51.284 -43 54 13.55   11.83 11.33 10.62 11.9 ~ 920 2
6 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4

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