On the fueling of massive black holes and the properties of their host spheroids
Author | dc.contributor.author | Escala, Andrés | |
Admission date | dc.date.accessioned | 2009-03-31T12:46:04Z | |
Available date | dc.date.available | 2009-03-31T12:46:04Z | |
Publication date | dc.date.issued | 2006-09-01 | |
Cita de ítem | dc.identifier.citation | ASTROPHYSICAL JOURNAL Volume: 648 Issue: 1 Pages: L13-L16 Part: Part 2 Published: SEP 1 2006 | en |
Identifier | dc.identifier.issn | 0004-637X | |
Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/124850 | |
Abstract | dc.description.abstract | We study the relation between nuclear massive black holes and their host spheroid gravitational potential. Using simple models, we analyze how gas is expected to be transported in the nuclear regions of galaxies. When we couple it with the expected gas lifetime given by the Kennicutt-Schmidt Law, this naturally leads to the "M-BH-bulge virial mass" and "M-BH-sigma" relations. | en |
Lenguage | dc.language.iso | en | en |
Publisher | dc.publisher | UNIV CHICAGO PRESS | en |
Keywords | dc.subject | BH-SIGMA RELATION | en |
Título | dc.title | On the fueling of massive black holes and the properties of their host spheroids | en |
Document type | dc.type | Artículo de revista |
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