English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/110542
Compartir / Impacto:
Estadísticas
Add this article to your Mendeley library MendeleyBASE
Citado 3 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 bibText (RIS)Exportar csv (RIS)
Título

Investigating the radio-loud phase of broad absorption line quasars

Autor Bruni, G.; González-Serrano, José Ignacio ; Pedani, M.; Benn, Chris; Mack, K. H.; Holt, J.; Montenegro-Montes, F. M.; Jiménez-Luján, F.
Palabras clave Galaxies: evolution
Galaxies: active
Quasars: absorption lines
Radio continuum: galaxies
Fecha de publicación 2014
EditorEDP Sciences
Citación Astronomy and Astrophysics 569: A87 (2014)
Resumen[Context]: Broad absorption lines (BALs) are present in the spectra of ~20% of quasars (QSOs); this indicates fast outflows (up to 0.2c) that intercept the observer's line of sight. These QSOs can be distinguished again into radio-loud (RL) BAL QSOs and radio-quiet (RQ) BAL QSOs. The first are very rare, even four times less common than RQ BAL QSOs. The reason for this is still unclear and leaves open questions about the nature of the BAL-producing outflows and their connection with the radio jet. [Aims]: We explored the spectroscopic characteristics of RL and RQ BAL QSOs with the aim to find a possible explanation for the rarity of RL BAL QSOs. [Methods]: We identified two samples of genuine BAL QSOs from SDSS optical spectra, one RL and one RQ, in a suitable redshift interval (2.5 < z < 3.5) that allowed us to observe the Mg ii and Hβ emission lines in the adjacent near-infrared (NIR) band. We collected NIR spectra of the two samples using the Telescopio Nazionale Galileo (TNG, Canary Islands). By using relations known in the literature, we estimated the black-hole mass, the broad-line region radius, and the Eddington ratio of our objects and compared the two samples. [Results]: We found no statistically significant differences from comparing the distributions of the cited physical quantities. This indicates that they have similar geometries, accretion rates, and central black-hole masses, regardless of whether the radio-emitting jet is present or not. [Conclusions]: These results show that the central engine of BAL QSOs has the same physical properties with and without a radio jet. The reasons for the rarity of RL BAL QSOs must reside in different environmental or evolutionary variables.
Versión del editorhttp://dx.doi.org/10.1051/0004-6361/201424424
URI http://hdl.handle.net/10261/110542
DOI10.1051/0004-6361/201424424
Identificadoresdoi: 10.1051/0004-6361/201424424
e-issn: 1432-0746
issn: 0004-6361
Aparece en las colecciones: (IFCA) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
Investigating the radio-loud.pdf916,6 kBAdobe PDFVista previa
Visualizar/Abrir
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.