MNRAS 467, 2504–2516 (2017) doi:10.1093/mnras/stx224 Advance Access publication 2017 January 27
Unveiling the AGN in IC 883: discovery of a parsec-scale radio jet
C. Romero-Canizales,˜ 1,2,3‹ A. Alberdi,4‹ C. Ricci,2‹ P. Arevalo,´ 5 M. A.´ Perez-Torres,´ 4,6† J. E. Conway,7 R. J. Beswick,8 M. Bondi,9 T. W. B. Muxlow,8 M. K. Argo,8,10 F. E. Bauer,1,2,11,12 A. Efstathiou,13 R. Herrero-Illana,4,14 S. Mattila15 andS.D.Ryder16 1Millennium Institute of Astrophysics, 7500011 Santiago, Chile 2Instituto de Astrof´ısica, Facultad de F´ısica, Pontificia Universidad Catolica´ de Chile, Casilla 306, Santiago 22, Chile 3Nucleo´ de Astronom´ıa de la Facultad de Ingenier´ıa y Ciencias, Universidad Diego Portales, Av. Ejercito´ 441, Santiago, Chile 4Instituto de Astrof´ısica de Andaluc´ıa – CSIC, PO Box 3004, E-18080 Granada, Spain 5Instituto de F´ısica y Astronom´ıa, Facultad de Ciencias, Universidad de Valpara´ıso, Gran Bretana˜ No. 1111, Playa Ancha, 2360102 Valpara´ıso, Chile 6Departamento de F´ısica Teorica, Facultad de Ciencias, Universidad de Zaragoza, E-50009 Zaragoza, Spain 7Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden 8Jodrell Bank Centre for Astrophysics, The University of Manchester, Oxford Rd, Manchester M13 9PL, UK 9Osservatorio di Radioastronomia–INAF, Bologna, via P. Gobetti 101, I-40129 Bologna, Italy 10Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK 11Centro de Astroingenier´ıa, Facultad de F´ısica, Pontificia Universidad Catolica´ de Chile, Casilla 306, Santiago 22, Chile 12Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, CO 80301, USA 13School of Sciences, European University Cyprus, Diogenes Street, Engomi, 1516 Nicosia, Cyprus 14European Southern Observatory (ESO), Alonso de Cordova´ 3107, Vitacura, Casilla 19001, Santiago de Chile, Chile 15Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Vais¨ al¨ antie¨ 20, FI-21500 Piikkio,¨ Finland 16Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia
Accepted 2017 January 23. Received 2017 January 23; in original form 2016 June 29
ABSTRACT IC 883 is a luminous infrared galaxy (LIRG) classified as a starburst-active galactic nucleus (AGN) composite. In a previous study, we detected a low-luminosity AGN (LLAGN) radio candidate. Here, we report on our radio follow-up at three frequencies that provides direct and unequivocal evidence of the AGN activity in IC 883. Our analysis of archival X-ray data, together with the detection of a transient radio source with luminosity typical of bright supernovae, gives further evidence of the ongoing star formation activity, which dominates the energetics of the system. At sub-parsec scales, the radio nucleus has a core-jet morphol- ogy with the jet being a newly ejected component showing a subluminal proper motion of 0.6–1 c. The AGN contributes less than 2 per cent of the total IR luminosity of the system. The corresponding Eddington factor is ∼10−3, suggesting this is a low-accretion rate engine, as often found in LLAGNs. However, its high bolometric luminosity (∼1044 erg s−1) agrees better with a normal AGN. This apparent discrepancy may just be an indication of the transi- tion nature of the nucleus from a system dominated by star formation, to an AGN-dominated system. The nucleus has a strongly inverted spectrum and a turnover at ∼4.4 GHz, thus qual- 28 −1 −1 ifying as a candidate for the least luminous (L5.0 GHz ∼ 6.3 × 10 erg s Hz ) and one of the youngest (∼3 × 103 yr) gigahertz-peaked spectrum (GPS) sources. If the GPS origin for the IC 883 nucleus is confirmed, then advanced mergers in the LIRG category are potentially key environments to unveil the evolution of GPS sources into more powerful radio galaxies. Key words: galaxies: active – galaxies: individual: IC 883 – galaxies: jets – galaxies: nuclei – " radio continuum: galaxies – X-rays: galaxies.