Tracing the merger-driven evolution of active galaxies using the CJF sample

Details Tracing the merger-driven evolution of active galaxies using the CJF sample Tracing the merger-driven evolution of active galaxies using the CJF sample

2010-05-12

arxiv.org/abs/1005.2177v2

A&A 519, A62 (2010)

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

18 pages, 6 figures, accepted for publication in A&A (updated to match proofs)

Scientific paper

10.1051/0004-6361/200913550

In the context of the evolution of large structures in the Universe, it is unclear whether active galaxies are a phase which each galaxy undergoes, and what is the importance of the evolution of black holes in their centers. Binary black hole (BBH) systems could play a key role in our understanding of the above question. We investigate the Caltech-Jodrell Bank flat-spectrum (CJF) sample for evidence in favor of the merger-driven evolution scheme of active galaxies and search tracer-systems of AGN evolution and possible indications of BBH candidates. We discuss the validity and ambiguity of such indications and formulate a set of selection criteria for the detection of such systems. We conduct an extensive literature search for all available multi-wavelength information, concentrating on the optical and infrared regime, in addition to morphological information of the CJF sources. We analyze the statistics of this sample, in terms of these properties. We find 1 ULIRG (Mrk 231) included in the CJF, prototype of a transitory system. In total 28.6% of the CJF sources with z<0.4 are distorted or have a companion. Given the unbiased sample used here, this provides strong evidence for the ubiquity of the merger phenomenon in the context of active galaxies. We find a correlation between the radio and the near-infrared luminosity for the high-luminosity sources, interpreted in the context of the interplay between a star-formation and AGN component. We find a connection between variability and evolutionary transitory systems, as selected through their near-infrared colors. We select 28 sources that trace the different evolution phases of an AGN, as well as a number of the most promising BBH candidates. We find 4 sources with almost periodical variability in the optical and radio on similar timescales.

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