The nuclear and extended mid-infrared emission of Seyfert galaxies

I. García-Bernete, C. Ramos Almeida, J. A. Acosta-Pulido, A. Alonso-Herrero, O. González-Martín, A. Hernán-Caballero, M. Pereira-Santaella, N. A. Levenson, C. Packham, E. S. Perlman, K. Ichikawa, P. Esquej, T. Díaz-Santos

Research output: Contribution to journalArticlepeer-review

12 Citations (Scopus)

Abstract

We present subarcsecond resolution mid-infrared (MIR) images obtained with 8-10 m-class ground-based telescopes of a complete volume-limited (DL < 40 Mpc) sample of 24 Seyfert galaxies selected from the Swift/Burst Alert Telescope nine month catalogue. We use those MIR images to study the nuclear and circumnuclear emission of the galaxies. Using different methods to classify the MIR morphologies on scales of ~400 pc, we find that the majority of the galaxies (75-83 per cent) are extended or possibly extended and 17-25 per cent are pointlike. This extended emission is compact and it has low surface brightness compared with the nuclear emission, and it represents, on average, ~30 per cent of the total MIR emission of the galaxies in the sample. We find that the galaxies whose circumnuclear MIR emission is dominated by star formation (SF) show more extended emission (650 ± 700 pc) than active galactic nuclei (AGN)-dominated systems (300 ± 100 pc). In general, the galaxies with pointlike MIR morphologies are face-on or moderately inclined (b/a ~ 0.4-1.0), and we do not find significant differences between the morphologies of Sy1 and Sy2. We used the nuclear and circumnuclear fluxes to investigate their correlation with different AGN and SF activity indicators. We find that the nuclear MIR emission (the inner ~70 pc) is strongly correlated with the X-ray emission (the harder the X-rays the better the correlation) and with the [OIV] λ25.89 μm emission line, indicating that it is AGN-dominated. We find the same results, although with more scatter, for the circumnuclear emission, which indicates that the AGN dominates the MIR emission in the inner ~400 pc of the galaxies, with some contribution from SF.

Original languageEnglish
Pages (from-to)3531-3555
Number of pages25
JournalMonthly Notices of the Royal Astronomical Society
Volume463
Issue number4
DOIs
Publication statusPublished - 2016 Dec 21
Externally publishedYes

Keywords

  • Galaxies: Seyfert
  • Galaxies: active
  • Galaxies: nuclei
  • Galaxies: photometry
  • Infrared: galaxies
  • Techniques: high angular resolution

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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