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Paper detail

Black hole growth and host galaxy morphology

We use data from large surveys of the local Universe (SDSS+Galaxy Zoo) to show that the galaxy-black hole connection is linked to host morphology at a fundamental level. The fraction of early-type galaxies with actively growing black holes, and therefore the AGN duty cycle, declines significantly with increasing black hole mass. Late-type galaxies exhibit the opposite trend: the fraction of actively growing black holes increases with black hole mass.

preprint2010arXivOpen access
Kevin SchawinskiC. Megan UrryShanil ViraniPaolo CoppiSteven P. BamfordEzequiel TreisterChris J. LintottMarc SarziWilliam C. KeelSugata KavirajCarolin N. CardamoneKaren L. MastersNicholas P. Rossthe Galaxy Zoo Team
astro-ph.CO
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Kevin SchawinskiC. Megan UrryShanil ViraniPaolo CoppiSteven P. BamfordEzequiel TreisterChris J. LintottMarc SarziWilliam C. KeelSugata KavirajCarolin N. CardamoneKaren L. MastersNicholas P. Rossthe Galaxy Zoo Team

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