Black Hole Growth and Host Galaxy Morphology

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dc.contributor.author Schawinski, Kevin
dc.contributor.author Urry, C. Megan
dc.contributor.author Virani, Shanil
dc.contributor.author Coppi, Paolo
dc.contributor.author Bamford, Steven P.
dc.contributor.author Treister, Ezequiel
dc.contributor.author Lintott, Chris J.
dc.contributor.author Sarzi, Marc
dc.contributor.author Keel, William C.
dc.contributor.author Kaviraj, Sugata
dc.contributor.author Cardamone, Carolin N.
dc.contributor.author Masters, Karen L.
dc.contributor.author Ross, Nicholas P.
dc.contributor.author Galaxy Zoo Team
dc.date.accessioned 2018-09-24T20:04:18Z
dc.date.available 2018-09-24T20:04:18Z
dc.date.issued 2010
dc.identifier.citation Schirmer, M., et al. (2009): Black Hole Growth and Host Galaxy Morphology. Proceedings of the International Astronomical Union, 5(267). DOI: https://doi.org/10.1017/S1743921310006964 en_US
dc.identifier.uri http://ir.ua.edu/handle/123456789/3956
dc.description.abstract 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. en_US
dc.format.mimetype application/pdf en_US
dc.relation.isformatof conferences en_US
dc.relation.ispartof International Astronomical Union. Symposium (267 : 2009 : Rio De Janeiro, Brazil) en_US
dc.subject galaxies: evolution en_US
dc.subject galaxies: Seyfert en_US
dc.subject galaxies: active en_US
dc.title Black Hole Growth and Host Galaxy Morphology en_US
dc.type text en_US


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