Query : 2018A&A...610A..74K

2018A&A...610A..74K - Astronomy and Astrophysics, volume 610A, 74-74 (2018/2-1)

Far-infrared photometry of OJ 287 with the Herschel Space Observatory.


Abstract (from CDS):

Context. The blazar OJ 287 has shown a ~=12 year quasi-periodicity over more than a century, in addition to the common properties of violent variability in all frequency ranges. It is the strongest known candidate to have a binary singularity in its central engine.
Aim. We aim to better understand the different emission components by searching for correlated variability in the flux over four decades of frequency measurements.
Methods. We combined data at frequencies from the millimetric to the visible to characterise the multifrequency light curve in April and May 2010. This includes the only photometric observations of OJ 287 made with the Herschel Space Observatory: five epochs of data obtained over 33 days at 250, 350, and 500µm with Herschel-SPIRE.
Results. Although we find that the variability at 37GHz on timescales of a few weeks correlates with the visible to near-IR spectral energy distribution, there is a small degree of reddening in the continuum at lower flux levels that is revealed by the decreasing rate of decline in the light curve at lower frequencies. However, we see no clear evidence that a rapid flare detected in the light curve during our monitoring in the visible to near-IR light curve is seen either in the Herschel data or at 37GHz, suggesting a low-frequency cut-off in the spectrum of such flares.
Conclusions. We see only marginal evidence of variability in the observations with Herschel over a month, although this may be principally due to the poor sampling. The spectral energy distribution between 37GHz and the visible can be characterised by two components of approximately constant spectral index: a visible to far-IR component of spectral index α=-0.95, and a far-IR to millimetric spectral index of α=-0.43. There is no evidence of an excess of emission that would be consistent with the 60 µmdust bump found in many active galactic nuclei.

Abstract Copyright: © ESO 2018

Journal keyword(s): Galaxies - BL Lacertae objects: individual: OJ 287

VizieR on-line data: <Available at CDS (J/A+A/610/A74): photom.dat>

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
1 3C 84 Sy2 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4003 3
2 QSO J0854+2006 BLL 08 54 48.8749846272 +20 06 30.639583620   15.91 15.43 15.56   ~ 2326 1
3 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7180 3
4 NAME Her B Sy1 16 42 58.80997043 +39 48 36.9939552   16.81 16.59 16.84   ~ 1723 2
5 NGC 7027 PN 21 07 01.571952 +42 14 10.47120   10.358 8.831 10.157   ~ 2456 1
6 NAME BL Lac BLL 22 02 43.2913536816 +42 16 39.979416792   15.66 14.72     ~ 2258 1

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