Por favor, use este identificador para citar o enlazar a este item:
http://hdl.handle.net/10261/3978
COMPARTIR / EXPORTAR:
SHARE CORE BASE | |
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE | |
Campo DC | Valor | Lengua/Idioma |
---|---|---|
dc.contributor.author | Page, Matt | - |
dc.contributor.author | Stevens, J. A. | - |
dc.contributor.author | Mittaz, J. P. D. | - |
dc.contributor.author | Carrera, Francisco J. | - |
dc.date.accessioned | 2008-05-04T18:55:01Z | - |
dc.date.available | 2008-05-04T18:55:01Z | - |
dc.date.issued | 2002-02-05 | - |
dc.identifier.citation | Science 294(5551): 2516-2518 (2001) | en_US |
dc.identifier.issn | 0036-8075 | - |
dc.identifier.uri | http://hdl.handle.net/10261/3978 | - |
dc.description.abstract | The correlation, found in nearby galaxies, between black hole mass and stellar bulge mass implies that the formation of these two components must be related. Here we report submillimeter photometry of eight x-ray absorbed active galactic nuclei which have luminosities and redshifts characteristic of the sources that produce the bulk of the accretion luminosity in the universe. The four sources with the highest redshifts are detected at 850 microns, with flux densities between 5.9 and 10.1 milliJanskies, and hence are ultraluminous infrared galaxies. Interpreting the submillimeter flux as emission from dust heated by starbursts, these results suggest that the majority of stars in spheroids were formed at the same time as their central black holes built up most of their mass by accretion, accounting for the observed demography of massive black holes in the local universe. The skewed rate of submillimeter detection with redshift is consistent with a high redshift epoch of star formation in radio quiet active galactic nuclei, similar to that seen in radio galaxies. | en_US |
dc.format.extent | 128877 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | en_US |
dc.publisher | American Association for the Advancement of Science | en_US |
dc.relation.isversionof | Preprint | - |
dc.rights | openAccess | en_US |
dc.subject | Black holes | en_US |
dc.subject | Stellar bulges | en_US |
dc.subject | Mass correlation | en_US |
dc.subject | Accretion luminosity | en_US |
dc.subject | Submillimeter flux | en_US |
dc.subject | Astrophysics | en_US |
dc.title | Submillimeter evidence for the coeval growth of massive black holes and galaxy bulges | en_US |
dc.type | artículo | en_US |
dc.identifier.doi | 10.1126/science.1065880 | - |
dc.description.peerreviewed | Peer reviewed | en_US |
dc.relation.publisherversion | http://dx.doi.org/10.1126/science.1065880 | - |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.openairetype | artículo | - |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
Aparece en las colecciones: | (IFCA) Artículos |
Ficheros en este ítem:
Fichero | Descripción | Tamaño | Formato | |
---|---|---|---|---|
0202102v1.pdf | 260,17 kB | Adobe PDF | Visualizar/Abrir |
CORE Recommender
SCOPUSTM
Citations
82
checked on 09-abr-2024
WEB OF SCIENCETM
Citations
84
checked on 21-feb-2024
Page view(s)
395
checked on 21-abr-2024
Download(s)
216
checked on 21-abr-2024
Google ScholarTM
Check
Altmetric
Altmetric
NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.