Astronomers discovered eight buried dual AGN candidates, the largest sample of hidden accreting supermassive black holes in late stage galaxy mergers, selected using NASA's Wide-Field Infrared Survey Explorer (WISE) space telescope.

This result will be presented by graduate student Ryan Pfeifle of George Mason University (Fairfax, Virginia, USA) at the annual meeting of the European Astronomical Society EWASS 2019, in Lyon, France, on Friday, 28 June.

Observational campaigns and theoretical studies have shown both that supermassive black holes (SMBHs) reside at the centers of most galaxies and that galaxy interactions are ubiquitous in the universe. As a result, galaxies grow and evolve hierarchically through collisions, which also fuel and consequently grow the SMBHs at their centers.

Late-stage mergers should in fact host dual accreting SMBHs, or active galactic nuclei (AGN) - unambiguous evidence for an ongoing merger - with pair separations smaller than 10 kpc and are predicted to facilitate the most rapid growth of the black holes. Decades of observational campaigns have demonstrated, however, the exceeding rarity of dual accreting SMBHs.

Not only do the existence, frequency, and accretion rates of such dual AGN systems have important astrophysical implications on the formation and growth of SMBHs and their connection to the host galaxies in which they reside, they are the precursors of SMBH mergers, which will be the most titanic gravitational wave events in the universe - a topic that is of current interest.

In a follow-up study the international team of scientists also reports - using high-spatial resolution X-ray, near-IR, and optical spectroscopic diagnostics - a case of a triplet of accreting supermassive black holes with mutual separations < 10 kiloparsecs (= 33,000 light-years) in the advanced merger SDSS J084905.51+111447.2.

The dynamics of a triple massive black hole system can greatly shorten the merger timescale for two black holes.

Ryan Pfeifle explains: "The discovery suggests that this may be an important mechanism for driving the binary black hole inspiral and producing sources of gravitational waves."

In addition, triple interactions can result in slingshot ejections of one of the black holes with velocities high enough to escape the host resulting in either ejected or wandering supermassive black holes.

Pfeifle concludes: "The results of our study demonstrates the true power of mid-infrared selection: it can select cases of dual AGN candidates that would be missed by optical selection techniques, and it now offers a method through which we can preselect triple mergers to try and find more triple AGN."

This work utilized data products from the Wide-Field Infrared Survey Explorer (WISE), the Sloan Digital Sky Survey (SDSS), the Chandra X-ray Observatory (CXO), the Large Binocular Telescope Observatory (LBTO), the X-ray Multi-Mirror Mission (XMM-Newton), the Nuclear Spectroscopic Telescope Array (NuSTAR), and the Hubble Space Telescope (HST).

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Detection of powerful winds driven by a supermassive black hole
Washington DC (SPX) Jun 10, 2019
The supermassive black holes in the centres of many galaxies seem to have a basic influence on their evolution. This happens during a phase in which the black hole is consuming the material of the galaxy in which it resides at a very high rate, growing in mass as it does so. During this phase we say that the galaxy has an active nucleus (AGN, for active galactic nucleus). The effect that this activity has on the host galaxy is known as AGN feedback, and one of its properties are galactic winds: th ... read more