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Black Hole Growth and Host Galaxy Morphology

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dc.contributor.authorSchawinski, Kevin
dc.contributor.authorUrry, C. Megan
dc.contributor.authorVirani, Shanil
dc.contributor.authorCoppi, Paolo
dc.contributor.authorBamford, Steven P.
dc.contributor.authorTreister, Ezequiel
dc.contributor.authorLintott, Chris J.
dc.contributor.authorSarzi, Marc
dc.contributor.authorKeel, William C.
dc.contributor.authorKaviraj, Sugata
dc.contributor.authorCardamone, Carolin N.
dc.contributor.authorMasters, Karen L.
dc.contributor.authorRoss, Nicholas P.
dc.contributor.authorGalaxy Zoo Team
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.date.accessioned2018-09-24T20:04:18Z
dc.date.available2018-09-24T20:04:18Z
dc.date.issued2010
dc.description.abstractWe 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.mimetypeapplication/pdf
dc.identifier.citationSchirmer, 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
dc.identifier.doi10.1017/S1743921310006964
dc.identifier.urihttp://ir.ua.edu/handle/123456789/3956
dc.relation.isformatofconferences
dc.relation.ispartofInternational Astronomical Union. Symposium (267 : 2009 : Rio De Janeiro, Brazil)
dc.subjectgalaxies: evolution
dc.subjectgalaxies: Seyfert
dc.subjectgalaxies: active
dc.titleBlack Hole Growth and Host Galaxy Morphologyen_US
dc.typetext

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