2024A&A...682A..18M


Query : 2024A&A...682A..18M

2024A&A...682A..18M - Astronomy and Astrophysics, volume 682A18 (2024/2-1)

A comparison of compact, presumably young with extended, evolved radio active galactic nuclei.

MEUSINGER H. and MHASKEY M.

Abstract (from CDS):

Context. The triggering and evolution of active galactic nuclei (AGNs) and the interaction of the AGN with its host galaxy is an important topic in extragalactic astrophysics. Radio sources with peaked spectra (peaked spectrum sources, PSS) and compact symmetric objects (CSO) are powerful, compact, and presumably young AGNs and therefore particularly suitable to study aspects of the AGN-host connection.
Aims. We use a statistical approach to investigate properties of a PSS-CSO sample that are related to host galaxies and could potentially shed light on the link between host galaxies and AGNs. The main goal is to compare the PSS-CSO sample with a matching comparison sample of extended sources (ECS) to see if the two have significant differences.
Methods. We analysed composite spectra, diagnostic line diagrams, multi-band spectral energy distributions (MBSEDs), star formation (SF) indicators, morphologies, and cluster environments for a sample of 121 PSSs and CSOs for which spectra are available from the Sloan Digital Sky Survey (SDSS). The statistical results were compared with those of the ECS sample, where we generally considered the two subsamples of quasi-stellar objects (QSOs) and radio galaxies separately. The analysis is based on a large set of archival data in the spectral range from the ultraviolet to mid-infrared.
Results. We find significant differences between the PSS-CSO and the ECS sample. In particular, we find that the ECS sample has a higher proportion of passive galaxies with a lower star formation activity. This applies to both sub-samples (QSOs or radio galaxies) as well as to the entire sample. The star formation rates of the PSS-CSO host galaxies with available data are typically in the range ∼0 to 5 ℳ⊙ yr–1, and the stellar masses are in the range 3 × 1011 to 1012 ℳ⊙. Secondly, in agreement with previous results, we find a remarkably high proportion of PSS-CSO host galaxies with merger signatures. The merger fraction of the PSS-CSO sample is 0.61 ± 0.07, which is significantly higher than that of the comparison sample (0.15 ± 0.06). We suggest that this difference can be explained by assuming that the majority of the PSSs and CSOs cannot evolve to extended radio sources and are therefore not represented in our comparison sample.

Abstract Copyright: © The Authors 2024

Journal keyword(s): galaxies: interactions - radio continuum: galaxies - galaxies: evolution - galaxies: nuclei - quasars: general - galaxies: active

VizieR on-line data: <Available at CDS (J/A+A/682/A18): tablec1.dat tablec2.dat>

Status at CDS : All or part of tables of objects will be ingested in SIMBAD with priority 1.

Simbad objects: 97

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Number of rows : 97
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 ICRF J002225.4+001456 Sy2 00 22 25.42584644 +00 14 56.1630395   21.1       ~ 125 1
2 4C 00.03 Sy2 00 28 33.4223118840 +00 55 11.003002176   18.69 18.17     ~ 36 1
3 ICRF J002914.2+345632 Sy2 00 29 14.24247204 +34 56 32.2470345   20.2       ~ 145 1
4 MCG-06-02-022a EmG 00 37 41.1133192392 -33 42 58.515101748   19.26   18.52   ~ 314 1
5 PKS 0054+018 rG 00 57 27.8890472640 +02 09 34.687276344           ~ 18 1
6 LBQS 0056-0009 Bla 00 59 05.5147782072 +00 06 51.620377428   18.07 17.89 16.9   ~ 300 1
7 3C 49 rG 01 41 09.161 +13 53 28.07   22.327 20.920 20.876   ~ 189 1
8 4C -00.12 QSO 02 25 07.9319769264 -00 35 32.987872212   19.98 19.36     ~ 85 1
9 ICRF J050258.4+251625 Sy2 05 02 58.47476282 +25 16 25.2757175   20       ~ 187 1
10 NVSS J073050+445600 rG 07 30 50.6685924696 +44 56 00.852055872           ~ 13 1
11 3C 186 QSO 07 44 17.4720658920 +37 53 17.250697320   17.5 18.14 17.2   ~ 339 1
12 FIRST J074919.2+200750 rG 07 49 19.084 +20 07 53.71           ~ 5 0
13 NVSS J075530+520450 rG 07 55 29.952 +52 04 50.60           ~ 14 1
14 6C 075246+502502 Sy2 07 56 28.7987936304 +50 17 16.355451696           ~ 34 1
15 2MASX J07575670+3959363 Sy2 07 57 56.7148709832 +39 59 36.104570412           ~ 47 1
16 3C 190 QSO 08 01 33.5525166480 +14 14 42.813906612   21.07 20.26 18.972   ~ 249 2
17 4C 30.13 QSO 08 04 42.2368690344 +30 12 37.030825404   18.56 18.17     ~ 82 1
18 3C 191 QSO 08 04 47.9671662720 +10 15 23.746977252   18.65 18.40     ~ 295 2
19 4C 07.22 BLL 08 13 23.7541734000 +07 34 05.603579760   19.28 18.44     ~ 36 1
20 NVSS J082504+315957 rG 08 25 04.5713344080 +31 59 57.045409692           ~ 16 1
21 LEDA 2275964 Bla 08 31 39.8039 +46 08 00.775   18.94 18.07 13.6   ~ 38 1
22 87GB 083013.0+581348 Bla 08 34 11.1012882048 +58 03 21.404149128           ~ 27 1
23 7C 083313.50+441135.00 Sy2 08 36 37.8438240792 +44 01 09.576639372           ~ 26 1
24 FIRST J084856.5+013647 Sy2 08 48 56.574 +01 36 47.82   21.60 20.62     ~ 32 1
25 NVSS J085408+021315 rG 08 54 08.44463 +02 13 16.1865           ~ 9 1
26 4C 29.32 QSO 08 56 01.2281175480 +28 58 35.444537832   19.43 19.13     ~ 52 1
27 7C 085805.20+291331.00 Sy2 09 01 05.2614565176 +29 01 46.939089828   18.84 18.08 18.600   ~ 132 1
28 6C 090251+464619 Bla 09 06 15.53979871 +46 36 19.0241852   16.80 16.08     ~ 63 1
29 3C 216.0 Bla 09 09 33.49714902 +42 53 46.4821036   19.98 19.42 18.220   ~ 520 1
30 LEDA 26638 Sy1 09 24 05.3017245816 +14 10 21.513088308   19.28 18.47     ~ 33 1
31 3C 220.2 QSO 09 30 33.5408086368 +36 01 25.145487660   18.83 18.37     ~ 118 1
32 PMN J0934+0305 rG 09 34 30.6842444592 +03 05 45.337007472   18.5   17.3 16.50 ~ 20 2
33 9C J0936+3313 LIN 09 36 09.3738424789 +33 13 08.458026732       13.85   ~ 26 1
34 7C 093818.10+395820.00 Sy2 09 41 24.0268234920 +39 44 41.809159068   16.36 16.4     ~ 195 2
35 NVSS J094525+352103 rG 09 45 25.9005678048 +35 21 03.561543864   19.37 18.65     ~ 33 1
36 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
37 3C 237.0 rG 10 08 00.0529 +07 30 16.830   21       ~ 197 1
38 2MASX J10095550+1401547 LIN 10 09 55.5118948152 +14 01 54.287661108   19.92 19.04     ~ 33 1
39 NVSS J101251+403903 rG 10 12 51.77989 +40 39 03.4250           ~ 11 1
40 ACO 963 ClG 10 17 03.4 +39 02 56           ~ 414 0
41 [OWG93] ACO 0963-B GiC 10 17 13.8660939576 +39 01 31.450381212   20.18   17.92   ~ 6 0
42 7C 101416.50+391624.00 QSO 10 17 14.10808 +39 01 23.8294   22.83 20.64     ~ 58 1
43 QSO B1014+392 QSO 10 17 14.2463927856 +39 01 21.075140784   20.0       ~ 9 0
44 SDSS J101714.32+390116.9 G 10 17 14.32443 +39 01 16.9634           ~ 1 0
45 LEDA 2269259 LIN 10 26 18.2613111266 +45 42 29.389879543           ~ 19 1
46 Z 212-30 LIN 10 37 19.3424977080 +43 35 15.305053488   14.6       ~ 91 1
47 7C 103742.79+301338.00 LIN 10 40 29.9436842112 +29 57 57.795289452 19.85 16 16.05     ~ 53 1
48 NGC 3468 Bla 10 57 31.1758726801 +40 56 46.117028267   14.2       ~ 66 1
49 SDSS J113852.21+501602.3 QSO 11 38 52.214 +50 16 02.34           ~ 4 0
50 4C 46.23 QSO 11 43 39.600 +46 21 20.44   14.9       ~ 64 0
51 6C 114716+554640 Bla 11 50 00.16487 +55 28 20.8780       14.3   ~ 29 1
52 87GB 115453.8+433443 Sy1 11 57 27.6034274352 +43 18 06.331660632   18.76 18.33     ~ 44 1
53 NVSS J115919+464545 rG 11 59 19.974 +46 45 45.16           ~ 8 1
54 7C 120500.2+340922 BLL 12 07 32.930 +33 52 40.13   16.4       ~ 97 1
55 NVSS J120902+411559 rG 12 09 02.7905671200 +41 15 59.305654152           ~ 16 1
56 SDSS J121427.42+595814.8 QSO 12 14 27.4302976776 +59 58 14.834240076           ~ 12 0
57 6C 124156+410806 BLL 12 44 19.9682592720 +40 51 36.652030020     19.43     ~ 40 1
58 ICRF J124733.3+672316 Bla 12 47 33.32959326 +67 23 16.4488689           ~ 100 2
59 3C 277.3 BLL 12 54 12.0071453880 +27 37 33.952663740   15.94       ~ 379 1
60 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
61 4C 39.38 QSO 13 17 18.6358054464 +39 25 28.140463668   18.45 18.20     ~ 64 1
62 ICRF J131739.1+411545 Bla 13 17 39.1954 +41 15 45.621           ~ 54 1
63 4C 04.45 rG 13 24 19.676 +04 19 07.05   19.5       ~ 31 1
64 2MASX J13251331+3955536 Bla 13 25 13.3643889408 +39 55 53.245066404           ~ 19 0
65 7C 132816.2+252436 QSO 13 30 37.6960744824 +25 09 10.983105972   18.31 17.67     ~ 373 1
66 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
67 LEDA 2252383 SyG 13 40 35.2016635824 +44 48 17.398175508           ~ 25 1
68 4C 38.37 QSO 13 45 36.9420854112 +38 23 12.500014308     18.5     ~ 97 1
69 PKS 1345+12 Sy2 13 47 33.36161873 +12 17 24.2398927   19.28 18.44 15.718   ~ 652 2
70 2MASX J14005162+5216068 LIN 14 00 51.5814702864 +52 16 06.473503164           ~ 21 1
71 Mrk 668 BLL 14 07 00.39441712 +28 27 14.6901341   16.13 15.35 10.29   ~ 826 3
72 87GB 140732.1+361738 Sy1 14 09 42.4485402456 +36 04 15.887047296           ~ 25 1
73 NVSS J141327+550529 rG 14 13 27.222 +55 05 29.27           ~ 12 1
74 QSO B1413+135 BLL 14 15 58.81751033 +13 20 23.7128587   21.055 20.000 18.461   ~ 476 1
75 7C 142237.3+201352 QSO 14 24 56.9189790528 +20 00 26.360208360   18.09 17.65     ~ 132 1
76 6C 143339+510410 LIN 14 35 21.6699085551 +50 51 22.922806306           ~ 24 1
77 NVSS J144712+404745 rG 14 47 12.7625124264 +40 47 44.987437896           ~ 28 1
78 QSO B1509+054 Bla 15 11 41.26637844 +05 18 09.2590927   18.49 17.80 13.95   ~ 122 0
79 NVSS J152349+321350 rG 15 23 49.3424305752 +32 13 50.347922988           ~ 12 1
80 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
81 ICRF J154609.5+002624 Bla 15 46 09.53146317 +00 26 24.6145149   19.730 18.900 19.5   ~ 91 1
82 SDSS J154754.12+351842.2 QSO 15 47 54.12293 +35 18 42.2545           ~ 15 0
83 NVSS J155700+413108 rG 15 57 00.1763842848 +41 31 11.133624900           ~ 14 1
84 7C 155812.19+533918.00 Sy2 15 59 27.644 +53 30 52.05   19.68 18.86     ~ 25 1
85 4C 52.37 Sy1 16 02 46.3870735776 +52 43 58.675644984   18.50 17.76     ~ 45 1
86 NVSS J160335+380643 rG 16 03 35.1750934464 +38 06 42.808318776   18.0       ~ 11 1
87 NGC 6090 PaG 16 11 40.3 +52 27 21   14.0       ~ 446 1
88 4C 40.34 BLL 16 11 48.5301162024 +40 40 20.955442404           ~ 26 1
89 4C 36.27B BLL 16 18 23.5801033152 +36 32 01.810874112   20.16 19.67 18.7   ~ 26 1
90 3C 346.0 BLL 16 43 48.605 +17 15 49.43   17.2       ~ 270 1
91 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1734 2
92 NAME Super Antennae Sy2 19 31 21.4272801984 -72 39 21.442847832   17.39 16.37 14.65   ~ 318 3
93 ESO 285-19 G 20 29 31.9 -42 30 15   14.2       ~ 10 0
94 ESO 286-19 LIN 20 58 26.8183783008 -42 38 59.411838156   14.79 14.79 14.20   ~ 318 0
95 QSO B2134+0028 Bla 21 36 38.58632232 +00 41 54.2128562   17.30 17.08 17.02   ~ 580 2
96 2MASX J22502534+1419519 Sy1 22 50 25.3475290512 +14 19 52.095751140   17.28 16.97 17.243   ~ 210 1
97 NAME South America rG 22 51 49.27872 -17 52 24.0600   16.97       ~ 348 3

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