English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/3978
Compartir / Impacto:
Add this article to your Mendeley library MendeleyBASE
Citado 80 veces en Web of Knowledge®  |  Ver citas en Google académico
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar otros formatos: Exportar EndNote (RIS)Exportar EndNote (RIS)Exportar EndNote (RIS)
Título : Submillimeter Evidence for the Coeval Growth of Massive Black Holes and Galaxy Bulges
Autor : Page, M. J.; Stevens, J. A.; Mittaz, J. P. D.; Carrera, Francisco J.
Palabras clave : Black holes
Stellar bulges
Mass correlation
Accretion luminosity
Submillimeter flux
Fecha de publicación : 5-feb-2002
Editor: American Association for the Advancement of Science
Citación : Science 294 : 2516 (2001)
Resumen: 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.
Descripción : Originally published in Science Express as 10.1126/science.1065880 on November 1, 2001. Published in Science, 294, 2516. Also in Science Online: http://www.sciencemag.org/cgi/content/full/294/5551/2516
Versión del editor: http://dx.doi.org/10.1126/science.1065880
URI : http://hdl.handle.net/10261/3978
DOI: 10.1126/science.1065880
ISSN: 0036-8075
Aparece en las colecciones: (IFCA) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
0202102v1.pdf260,17 kBAdobe PDFVista previa
Mostrar el registro completo

NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.