2004ApJ...617..903W


Query : 2004ApJ...617..903W

2004ApJ...617..903W - Astrophys. J., 617, 903-914 (2004/December-3)

The fundamental plane evolution of active galactic nucleus host galaxies.

WOO J.-H., URRY C.M., LIRA P., VAN DER MAREL R.P. and MAZA J.

Abstract (from CDS):

We measured the stellar velocity dispersions of 15 active galactic nucleus (AGN) host galaxies at redshifts as high as ∼0.34. Combining these with published velocity dispersion measurements from the literature, we study the fundamental plane of AGN host galaxies and its evolution. BL Lac object hosts and radio galaxies seem to lie on the same fundamental plane as normal early-type galaxies. The evolution of the mass-to-light ratio of AGN host galaxies shows a similar trend to that observed in normal early-type galaxies, consistent with single-burst passive evolution models with formation redshifts z≳1. The lack of a significant difference between normal and AGN host galaxies in the fundamental plane supports the ``grand unification'' picture wherein AGNs are a transient phase in the evolution of normal galaxies. The black hole masses of BL Lac objects and radio galaxies, derived using the mass dispersion relation, are similar. The black hole mass is independent of BL Lac object type. The local black hole mass-host galaxy luminosity relation of our subsample at z<0.1 is similar to that of local normal and radio galaxies, but is less well defined at higher redshift owing to the luminosity evolution of the host galaxies.

Abstract Copyright:

Journal keyword(s): Black Hole Physics - Galaxies: BL Lacertae Objects: General - Galaxies: Active - Galaxies: Evolution - Galaxies: Formation - Galaxies: Quasars: General

Simbad objects: 25

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Number of rows : 25
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 QSO B0122+09 BLL 01 24 44.5398641328 +09 18 49.289559588     19.98 18.5   ~ 57 0
2 QSO B0145+138 BLL 01 48 29.7013033536 +14 02 17.848330656     17.90 16.7   ~ 45 0
3 QSO B0229+200 BLL 02 32 48.6148874688 +20 17 17.486717388   18.0 18.00     ~ 290 3
4 QSO B0331-362 BLL 03 33 12.2677895088 -36 19 46.662911112   19.94 18.0 17.99   ~ 59 0
5 2MASS J05313736+7121513 BLL 05 31 37.3913773368 +71 21 51.161254668     19.0     ~ 13 0
6 QSO B0548-322 BLL 05 50 40.5705144672 -32 16 16.484718648   16.07 15.5     ~ 386 1
7 6C 070609+591309 BLL 07 10 30.0683697888 +59 08 20.371772544   17.38 16.52 15.1   ~ 202 2
8 QSO B0829+047 BLL 08 31 48.8770033992 +04 29 39.086842884   17.10 16.4 14.55   ~ 442 2
9 Mrk 421 BLL 11 04 27.3140835504 +38 12 31.798495872   13.50 12.90 8.31   ~ 2540 1
10 6C 113337+702604 BLL 11 36 26.4090783600 +70 09 27.309071232   15.16 14.49 10.51   ~ 339 1
11 QSO B1212+078 BLL 12 15 10.9765816512 +07 32 04.676330688     16.0 14.8   ~ 89 1
12 PKS 1215-033 rG 12 17 55.2979512456 -03 37 23.249281512   19.336 18.9 19.177   ~ 19 1
13 LEDA 39531 BLL 12 18 27.7800402360 +01 02 37.335539616   17.40   17.012   ~ 32 0
14 PKS J1345-0156 rG 13 45 16.8665165568 -01 56 25.651411548   17.80       ~ 25 1
15 QSO B1514-24 BLL 15 17 41.8134049824 -24 22 19.482207024   15.13 14.00 13.95   ~ 704 3
16 4C 39.49 BLL 16 53 52.2160772976 +39 45 36.613228860 14.09 14.15 13.29 8.26   ~ 2037 2
17 6C 172704+501607 BLL 17 28 18.6242294352 +50 13 10.469553996   16.55 15.97 12.95   ~ 344 1
18 3C 371 BLL 18 06 50.6802916920 +69 49 28.109609256   14.77 14.22 11.39   ~ 820 2
19 QSO B1853+671 BLL 18 53 52.0667262720 +67 13 55.016841792     16.4 17.1   ~ 40 1
20 QSO B1959+650 BLL 19 59 59.8520303688 +65 08 54.652536492     12.8 11.21   ~ 557 2
21 QSO B2143+07 BLL 21 45 52.2999532008 +07 19 27.205685508     18.04 16   ~ 103 1
22 4C 04.77 BLL 22 04 17.6521146096 +04 40 02.027503020   16.20 15.2 10.2   ~ 188 2
23 QSO B2254+0727 BLL 22 57 17.3029968648 +07 43 12.297630108   17.07 16.36     ~ 291 1
24 QSO B2344+514 BLL 23 47 04.8372110928 +51 42 17.877513168     15.50 10.7   ~ 414 0
25 QSO B2356-309 BLL 23 59 07.9034996184 -30 37 40.671098544   18.414 16.44 16.795   ~ 275 1

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2022.09.26-08:26:33

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