Supermassive black hole hiding in a doughnut of dust confirms 30 year old theory

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Artist’s impression of the active galactic nucleus of Messier 77,  Credit: ESO/M. Kornmesser and L. Calçada
Artist’s impression of the active galactic nucleus of Messier 77, Credit: ESO/M. Kornmesser and L. Calçada

Aussie and international researchers have spotted a cloud of cosmic dust at the centre of a nearby galaxy hiding a supermassive black hole, a finding that confirms a 30 year old theory known as the Unified Model of Active Galactic Nuclei (AGN). Active galactic nuclei are high energy areas at the centre of some galaxies which are thought to be powered by supermassive black holes, but some shine much brighter than others. The Unified Model suggests that all AGNs have the same basic structure: a supermassive black hole surrounded by a thick ring of dust, and any differences are down to the angle at which we view the black hole and its thick ring from Earth. The researchers used high-resolution images of the galaxy NGC 1068 to reveal a doughnut-shaped dust cloud with a black hole at its centre  - features that match those expected by the unified model.

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From: Springer Nature

Astronomy: Confirming the ‘unified model’ of active galactic nuclei (N&V) *IMAGES*

Observations of the dense, obscuring dust surrounding a central black hole in a nearby galaxy provide confirmation of the unified model of active galactic nuclei. This conclusion is made through the analysis of high-resolution images of the galaxy, published in Nature this week. The images offer new opportunities to study active galactic nuclei.

Active galactic nuclei are energetic regions at the centre of some galaxies, thought to be powered by supermassive black holes. The light emitted by such nuclei produces spectral features relating to the region from which the light is emitted; distinct spectra have been used to split active galactic nuclei into two categories: type 1 or type 2 objects. However, the unified model suggests that this distinction arises because the line of sight may sometimes be obscured by a dusty torus-shaped cloud surrounding and feeding the central black hole.

Violeta Gámez Rosas and colleagues report observations that support this unified model. They obtain high-resolution images of the archetypal galaxy NGC 1068, from which the unified model was first established. They use an instrument called MATISSE, which combines the light of four European Southern Observatory telescopes, to get the best view of the active galactic nuclei. The analysis of the images and radio maps reveal the torus-shaped dust cloud and help to define its properties, which match those expected by the unified model. The authors also pinpoint the location of the black hole below the torus, which also fits the model.

Robert Antonucci, who helped to create the unified model, writes, “we can celebrate the fact that Gámez Rosas and colleagues’ study is the best proof yet that the unified model is correct,” in an accompanying News & Views article.

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Nature
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Organisation/s: The University of Sydney, Leiden University, The Netherlands
Funder: MATISSE was defined, funded and built in close collaboration with ESO, by a consortium composed of French (INSU-CNRS in Paris and OCA in Nice), German (MPIA, MPIfR and University of Kiel), Dutch (NOVA and University of Leiden), and Austrian (University of Vienna) institutes. The Conseil Départemental des Alpes-Maritimes in France, the Konkoly Observatory and Cologne University have also provided resources for the manufacture of the instrument. A thought goes to our two deceased OCA colleagues, Olivier Chesneau and Michel Dugué, with us at the origin of the MATISSE project, and with whom we shared many beautiful moments. V.G.R. was partially supported by the Netherlands Organisation for Scientific Research (NWO). J.H.L. acknowledges the support of the French government through the UCA JEDI Investment in the Future project managed by the National Research Agency (ANR) under the reference number ANR-15-IDEX-01.
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