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Investigating the radio-loud phase of broad absorption line quasars
Indexado
WoS WOS:000343092100123
Scopus SCOPUS_ID:84907513301
DOI 10.1051/0004-6361/201424424
Año 2014
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



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.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

Métricas Externas



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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Bruni, G. Mujer Max Planck Inst Radio Astron - Alemania
INAF Ist Radioastron - Italia
Max Planck Institute for Radio Astronomy - Alemania
Istituto Di Radioastronomia, Bologna - Italia
2 GONZALEZ-SERRANO, JOSE IGNACIO Hombre CSIC Univ Cantabria - España
Universidad de Cantabria - España
3 Pedani, M. - Istituto Nazionale di Astrofisica - España
Fundación Galileo Galilei - España
4 Benn, Chris Hombre Grupo de Telescopios Isaac Newton, España - España
Isaac Newton Group - España
5 Mack, K-H - INAF Ist Radioastron - Italia
Istituto Di Radioastronomia, Bologna - Italia
6 Holt, J. - Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos
Sterrewacht Leiden - Países Bajos
7 MONTENEGRO-MONTES, FRANCISCO MIGUEL Hombre ESO - Chile
European Southern Observatory Santiago - Chile
Observatorio Europeo Austral - Chile
8 Jimenez-Lujan, F. - Univ Cantabria - España
Universidad de Atacama - Chile
Universidad de Cantabria - España

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Origen de Citas Identificadas



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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 33.33 %
Citas No-identificadas: 66.67 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 33.33 %
Citas No-identificadas: 66.67 %

Financiamiento



Fuente
National Science Foundation
COST Action
Ohio State University
Spanish Ministerio de Ciencia e Innovación
Vanderbilt University
University of Tokyo
Yale University
Alfred P. Sloan Foundation
U.S. Department of Energy Office of Science
University of Arizona
Brazilian Participation Group
Brookhaven National Laboratory
Carnegie Mellon University
University of Florida
French Participation Group
German Participation Group
Harvard University
Instituto de Astrofisica de Canarias
Michigan State/Notre Dame/JINA Participation Group
Johns Hopkins University
Lawrence Berkeley National Laboratory
Max Planck Institute for Astrophysics
Max Planck Institute for Extraterrestrial Physics
New Mexico State University
New York University
Pennsylvania State University
University of Portsmouth
Princeton University
Spanish Participation Group
University of Utah
University of Virginia
University of Washington
European Cooperation in Science and Technology
University of Cambridge
Fondo Nacional de Ciencia Tecnología e Innovación

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Agradecimientos



Agradecimiento
The authors acknowledge financial support from the Spanish Ministerio de Ciencia e Innovacion under projects AYA2008-06311-C02-02 and AYA2011-29517-C03-02. Part of this work was supported by the COST Action MP0905 "Black Holes in a Violent Universe". Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundacion Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the participating institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
The authors acknowledge financial support from the Spanish Ministerio de Ciencia e Innovación under projects AYA2008-06311-C02-02 and AYA2011-29517-C03-02. Part of this work was supported by the COST Action MP0905 “Black Holes in a Violent Universe”. Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the participating institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.

Muestra la fuente de financiamiento declarada en la publicación.