The Origin Of The Relationship Between Black Hole Mass And Host Galaxy Bulge Luminosity

dc.contributor.utaustinauthorGaskell, C. Martinen
dc.creatorGaskell, C. M.en
dc.date.accessioned2015-04-16T14:47:46Zen
dc.date.available2015-04-16T14:47:46Zen
dc.date.issued2010-11en
dc.description.abstractThere is a strong decrease in scatter in the M(circle dot) - L(bulge) relationship with increasing luminosity and very little scatter for the most luminous galaxies. It is shown that this is a natural consequence of the substantial initial dispersion in the ratio of black hole mass to total stellar mass and of subsequent galaxy growth through hierarchical mergers. >Fine-tuning> through feedback between black hole growth and bulge growth is neither necessary nor desirable.en
dc.description.departmentAstronomyen
dc.identifier.citationC. Martin Gaskell. AIP Conference Proceedings 1294, 261 (Nov., 2010); doi: 10.1063/1.3518867en
dc.identifier.doi10.1063/1.3518867en
dc.identifier.issn0094-243Xen
dc.identifier.issn978-0-7354-0849-4en
dc.identifier.urihttp://hdl.handle.net/2152/29426en
dc.language.isoEnglishen
dc.relation.ispartofserialFirst Stars and Galaxies: Challenges for the Next Decadeen_US
dc.rightsAdministrative deposit of works to UT Digital Repository: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en
dc.subjectblack hole growthen
dc.subjectgalaxies: fundamental parametersen
dc.subjectgalaxies: nucleien
dc.subjectgalaxies: bulgesen
dc.subjectastronomy & astrophysicsen
dc.subjectphysics, applieden
dc.titleThe Origin Of The Relationship Between Black Hole Mass And Host Galaxy Bulge Luminosityen
dc.typeArticleen
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