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19 April 2024
 
  » arxiv » astro-ph/0102356

 Article overview


Monitoring of the optical and 2.5-11.7 micron spectrum and mid-IR imaging of the Seyfert 1 galaxy Mrk279 with ISO
The AGN Watch collaboration: M. Santos-Lleo ; J. Clavel ; B. Schulz ; B. Altieri ; P. Barr ; D. Alloin ; P. Berlind ; R. Bertram ; D.M. Crenshaw ; R.A. Edelson ; U. Giveon ; K. Horne ; J.P. Huchra ; S. Kaspi ; G.A. Kriss ; J.H. Krolik ; M.A. Malkan ; Yu.F. Malkov ; H. Netzer ; P.T. O’Brien ; B.M. Peterson ; et al ;
Date 21 Feb 2001
Subject astro-ph
AbstractMid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum. Contemporaneous optical photometric and spectrophotometric observations are also presented. The galaxy appears as a point-like source at the resolution of the ISOCAM instrument, 4-5". The 2.5-11.7 micron average spectrum of the nucleus in Mrk 279 shows a strong power law continuum with a spectral index alpha = -0.80+/-0.05 and weak PAH emission features. The Mrk 279 spectral energy distribution shows a mid-IR bump, which extends from 2 to 15-20 micron . The mid-IR bump is consistent with thermal emission from dust grains at a distance of >= 100 light-days. No significant variations of the mid-IR flux have been detected during our observing campaign, consistent with the relatively low amplitude (~10 % rms) of the optical variability during the campaign. The time delay for the Hbeta line emission in response to the optical continuum variations is 16.7 +5.3/5.6 days, consistent with previous measurements.
Source arXiv, astro-ph/0102356
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