Galaxies on a collision course may feed supermassive black holes

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Galaxies on a collision course may feed supermassive black holes
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New research seeks to reveal the secrets behind these celestial objects.

Observations of the nearby universe reveal an increasing fraction of active galactic nuclei with decreasing projected separation for close galaxy pairs, relative to control galaxies. This implies galaxy interactions play a role in enhancing AGN activity. However, the picture at higher redshift is less established, partly due to limited spectroscopic redshifts.

We combine spectroscopic surveys with photometric redshift probability distribution functions for galaxies in the CANDELS and COSMOS surveys, to produce the largest ever sample of galaxy pairs used in an AGN fraction calculation for cosmic noon or infrared-selected AGN in major or minor galaxy pairs. However, defining the most obscured AGN as those detected in the infrared but not in X-rays, we observe a trend of increasing obscured AGN enhancement at decreasing separations.

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