2005A&A...440..831K


C.D.S. - SIMBAD4 rel 1.7 - 2021.02.26CET19:48:54

2005A&A...440..831K - Astronomy and Astrophysics, volume 440, 831-843 (2005/9-4)

The luminous host galaxies of high redshift BL Lac objects.

KOTILAINEN J.K., HYVOENEN T. and FALOMO R.

Abstract (from CDS):

We present the first near-infrared Ks-band (2.1µm) imaging study of a sizeable sample of 13 high redshift (0.6<z<1.3) BL Lac objects in order to characterize the properties of their host galaxies. We are able to clearly detect the surrounding nebulosity in eight objects, and marginally in three others. In all the well resolved objects, we find that the host galaxy is well represented by a de Vaucouleurs r1/4 surface brightness law. In only two cases the object remains unresolved. These new observations represent in most cases the first detection of the host galaxy and taken together with previous optical studies of z >0.5 BL Lacs substantially increase the number of detected hosts (from ∼20 to ∼30). This dataset allows us to explore the evolution of BL Lac hosts from z∼1 to the present epoch. We find that the host galaxies of high redshift BL Lacs are large (average bulge scale length <R(e)≳7kpc) and similar to those hosting low redshift BL Lacs, indicating that there is no evolution in the host galaxy size. On the other hand, these host galaxies are very luminous (average <M(K)≥-27.9±0.7). They are ∼3mag brighter than the typical galaxy luminosity L*, and ∼1-1.5mag more luminous than brightest cluster galaxies at low redshift. They are also ∼1mag brighter than radio galaxies at low redshift and they appear to deviate from the K-z relationship of radio galaxies. On the other hand, these high luminosities agree with the few optical studies of high redshift BL Lacs and are similar to those of flat spectrum radio quasars studied by us in the near-infrared. The nuclear luminosity and the nucleus-galaxy luminosity ratio of the high redshift BL Lacs are much larger than those found for low redshift BL Lacs and similar to those observed in flat spectrum radio quasars at similar redshift. This mainly reflects the selection effects in the surveys and may be due to either an higher intrinsic nuclear luminosity, or due to enanched luminosity because of strong beaming. Contrary to what is observed in low redshift BL Lacs, the luminosities of the host galaxy and of the nucleus appear fairly well correlated, as expected from the black hole mass - bulge luminosity relationship found in nearby spheroids, if the nuclear emission works at the same regime. Our observations indicate that high redshift BL Lacs radiate with a wide range of power with respect to their Eddington luminosity, and this power is intermediate between the low level observed in nearby BL Lacs and the higher level occurring in luminous radio-loud quasars. The comparison with BL Lac host galaxies at lower redshift suggests that there is a ∼2mag brightening of the hosts. We argue that the large luminosity of the hosts is due to a strong selection effect in the surveys of BL Lacs that makes observable only the most luminous sources at z>0.5 and produces a correlation between the nuclear and the host luminosity that emerges at high redshift. However, this may also suggest a strong luminosity evolution which is inconsistent with a simple passive evolution of the stars in the host galaxies, and requires a contribution from recent star formation episodes that takes place at z>0.5.

Abstract Copyright:

Journal keyword(s): BL Lacertae objects: general - galaxies: active - galaxies: elliptical and lenticular, cD - galaxies: nuclei - galaxies: photometry - infrared: galaxies

Simbad objects: 14

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Number of rows : 14

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 QSO B0138-097 BLL 01 41 25.83215547 -09 28 43.6741894   16.94 16.55 17.21   ~ 249 3
2 QSO B0235+1624 BLL 02 38 38.93010 +16 36 59.2746   16.46 15.50 15.92   ~ 1412 2
3 7C 1308+3236 BLL 13 10 28.66387 +32 20 43.7831   15.61 15.24 17.91   ~ 760 1
4 QSO B1422+580 BLL 14 22 38.8818389583 +58 01 55.517270650   18.49 18.15 17.7   ~ 67 0
5 QSO B1517+656 BLL 15 17 47.5884450040 +65 25 23.284362137     15.9 16.7   ~ 103 1
6 QSO B1533+535 BLL 15 35 00.7964829745 +53 20 37.309526526   19.18 18.75 18.8   ~ 53 0
7 4C 14.60 BLL 15 40 49.49151734 +14 47 45.8848470   17.72 17.30 17.240   ~ 387 1
8 7C 1749+7006 BLL 17 48 32.8399653579 +70 05 50.768853537   17.46 17.01 15.48   ~ 394 1
9 8C 1803+784 BLL 18 00 45.6831135718 +78 28 04.017792333   16.4 16.4 15.46   ~ 675 1
10 4C 56.27 BLL 18 24 07.06837771 +56 51 01.4908371   18.9 18.4 16.48   ~ 447 1
11 QSO B2032+107 QSO 20 35 22.3341660153 +10 56 06.789797044   17.96 16.37 17.4   ~ 167 1
12 4C -02.81 BLL 21 34 10.30959643 -01 53 17.2387909   18.6 19.0 18.87   ~ 337 1
13 4C 02.54 QSO 22 09 32.8003861957 +02 18 40.916448378     19.0     ~ 33 1
14 [HNP96] PKS 0139-097 C G ~ ~           ~ 4 0

    Equat.    Gal    SGal    Ecl

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