2009A&A...502..457G


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.05CET21:16:06

2009A&A...502..457G - Astronomy and Astrophysics, volume 502, 457-472 (2009/8-1)

Resolving the mid-infrared cores of local Seyferts.

GANDHI P., HORST H., SMETTE A., HOENIG S., COMASTRI A., GILLI R., VIGNALI C. and DUSCHL W.

Abstract (from CDS):

We present new photometry of 16 local Seyferts including 6 Compton-thick sources in N-band filters around 12-µm, obtained with the VISIR instrument on the 8-m Very Large Telescope. The near-diffraction-limited imaging provides the least-contaminated core fluxes for these sources to date. Augmenting these with our previous observations and with published intrinsic X-ray fluxes, we form a total sample of 42 sources for which we find a strong mid-infrared: X-ray (12.3µm:2-10keV) luminosity correlation. Performing a physically-motivated subselection of sources in which the Seyfert torus is likely to be best-resolved results in the correlation LMIR∝LX1.11±0.07, with a reduction of the scatter in luminosities as compared to the full sample. Consideration of systematics suggests a range of 1.02-1.21 for the correlation slope. The mean 2-keV:12.3-µm spectral index (αIX) is found to be -1.10±0.01, largely independent of luminosity. Indirectly-computed 12-µm bolometric corrections range over ≃10-30 if a known luminosity trend of X-ray bolometric corrections is assumed. Comparison with ISO data spanning a wider luminosity range suggests that our correlation can be extended into the quasar regime. That unobscured, obscured, and Compton-thick sources all closely follow the same luminosity correlation has important implications for the structures of Seyfert cores. The typical resolution-limit of our imaging corresponds to ∼70pc at a median z=0.01, and we use the tightness of the correlation to place constraints on the dominance of any residual emission sources within these physical scales. An upper-limit for any contaminating star formation of ≃40% of the unresolved flux is inferred, on average. We suggest that uncontaminated mid-IR continuum imaging of AGN is an accurate proxy for their intrinsic power.

Abstract Copyright:

Journal keyword(s): galaxies: active - infrared: galaxies - X-rays: galaxies - galaxies: Seyfert - accretion, accretion disks

Simbad objects: 47

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Number of rows : 47

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 ESO 113-45 Sy1 01 23 45.7630391439 -58 48 20.811630442   14.08 13.83 13.34   ~ 787 0
2 NGC 526 Sy1 01 23 54.3778199024 -35 03 55.695504754   14.76 14.60 13.46   ~ 300 1
3 ESO 297-18 Sy2 01 38 37.141 -40 00 41.23   14.28   12.96   ~ 74 1
4 NGC 863 Sy1 02 14 33.5610949475 -00 46 00.180128181   14.48 13.81 17.9   ~ 594 0
5 M 77 GiP 02 42 40.771 -00 00 47.84 9.70 9.61 8.87 10.1 9.9 ~ 4180 2
6 NGC 1097 LIN 02 46 19.059 -30 16 29.68 10.46 9.97 9.48 8.72 9.8 ~ 1201 3
7 NAME Chandra Deep Field-South reg 03 32 28.0 -27 48 30           ~ 1859 1
8 2MASX J05210136-2521450 Sy2 05 21 01.3987198411 -25 21 45.269338983   15.47 14.75     ~ 438 0
9 ESO 5-4 Sy2 06 05 41.721 -86 37 55.02   13.55   11.88 12.2 ~ 130 0
10 ESO 428-14 Sy2 07 16 31.2067043371 -29 19 28.898984517   13.28 13.52 11.61   ~ 224 4
11 ESO 209-12 Sy1 08 01 57.9736077076 -49 46 42.394360438   15.31 15.3 13.78   ~ 66 0
12 NGC 3081 Sy2 09 59 29.5436045645 -22 49 34.748021329   13.06 13.55 11.67 12.1 ~ 422 0
13 ESO 263-13 Sy2 10 09 48.1881615625 -42 48 40.538299552   14.94 14.95 13.29   ~ 86 0
14 NGC 3281 Sy2 10 31 52.086 -34 51 13.40   12.62 14.02 11.17   ~ 326 0
15 NGC 3393 Sy2 10 48 23.467 -25 09 43.30   13.10 13.95 11.67 12.2 ~ 364 3
16 NGC 3783 Sy1 11 39 01.7095761008 -37 44 19.008597647   12.46 13.43 11.33 12.1 ~ 1500 0
17 NGC 4388 Sy2 12 25 46.820 +12 39 43.45 11.91 11.76 11.02     ~ 1218 2
18 NGC 4507 Sy2 12 35 36.6328010225 -39 54 33.661858548   12.95 13.54 11.70 12.4 ~ 446 0
19 M 58 SyG 12 37 43.597 +11 49 05.12 10.80 10.48 9.66     ~ 985 2
20 NGC 4593 Sy1 12 39 39.4435521178 -05 20 39.035028119   13.95 13.15     ~ 972 0
21 IC 3639 Sy2 12 40 52.8357581136 -36 45 21.046225445   13.01 13.50 11.87 12.7 ~ 228 1
22 ESO 323-32 Sy2 12 53 20.3092757460 -41 38 08.273024193   13.89 13.61 12.29   ~ 70 0
23 NGC 4941 Sy2 13 04 13.1053484000 -05 33 05.754194531   13.18 12.23 10.74   ~ 315 0
24 NGC 4992 Sy2 13 09 05.596 +11 38 02.85   14.6       ~ 98 0
25 MCG-03-34-064 Sy2 13 22 24.485 -16 43 42.09   14   13.16   ~ 269 2
26 NAME Centaurus A Sy2 13 25 27.61509104 -43 01 08.8056025   8.18 6.84 6.66   ~ 4077 3
27 NGC 5135 Sy2 13 25 44.059 -29 50 01.24   12.58 13.35 11.53 12.2 ~ 434 1
28 ESO 383-35 Sy1 13 35 53.7686909139 -34 17 44.139127597   13.89 13.61 8.9   ~ 1400 0
29 Mrk 463 Sy2 13 56 02.9 +18 22 18   14.8 14.22     ~ 356 2
30 NGC 5728 Sy2 14 42 23.928 -17 15 11.41   14.34 13.40     ~ 519 0
31 NGC 5995 Sy2 15 48 24.9486951203 -13 45 27.258674402   14.66 13.69 13.17   ~ 132 0
32 ESO 138-1 Sy2 16 51 20.2687785665 -59 14 04.287486933   14.35 13.63 13.02   ~ 113 0
33 NGC 6300 Sy2 17 16 59.473 -62 49 13.98   10.88 13.08 9.44 10.2 ~ 371 0
34 ESO 103-35 Sy2 18 38 20.3207055742 -65 25 39.142872479   14.75 14.53 13.24   ~ 282 0
35 ESO 141-55 Sy1 19 21 14.1471805047 -58 40 12.981632705   14.36 13.64 13.28   ~ 327 0
36 NGC 6814 Sy1 19 42 40.5857305428 -10 19 25.102133898   15.33 14.21 11.7 11.3 ~ 733 0
37 Mrk 509 Sy1 20 44 09.7504131334 -10 43 24.724854084   13.35 13.12 10.7   ~ 1150 0
38 IC 5063 Sy2 20 52 02.329 -57 04 07.60   12.92 13.60 11.30   ~ 564 1
39 Mrk 1513 Sy1 21 32 27.8163185343 +10 08 19.250705656   14.92 14.64     ~ 553 0
40 NGC 7172 Sy2 22 02 01.897 -31 52 11.60   12.72 13.61 11.15   ~ 480 1
41 NGC 7213 Sy1 22 09 16.2106632887 -47 10 00.082166299   10.97 12.08 10.50 10.6 ~ 606 0
42 LEDA 68751 Sy1 22 23 49.7 -02 06 13   16.93 15.77 16.02   ~ 442 2
43 NGC 7314 Sy1 22 35 46.1969940596 -26 03 01.574026329   11.62 13.11 10.61 11.4 ~ 512 0
44 NGC 7469 Sy1 23 03 15.674 +08 52 25.28 12.60 13.00 12.34     ~ 1919 3
45 2MASX J23083397+0521293 Sy2 23 08 33.9521188955 +05 21 29.763819747           ~ 136 0
46 NGC 7674 Sy2 23 27 56.6974755223 +08 46 44.238278540 13.84 13.92 13.23 12.64   ~ 648 4
47 NGC 7679 Sy2 23 28 46.670 +03 30 40.99   13.2       ~ 239 1

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2021.03.05-21:16:06

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