Dataciencia

Colección SciELO Chile

The effect of local and large-scale environments on nuclear activity and star formation

Indexado

WoS	WOS:000384722600089
Scopus	SCOPUS_ID:84978935156

DOI

10.1051/0004-6361/201628232

Año

2016

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The optical AGN phenomenon is related to cold gas accretion, while radio AGN are related to hot gas accretion. In this context, there is more cold gas, fuelling the central optical AGN, in isolated systems. Our results are in agreement with a scenario where cold gas accretion by secular evolution is the main driver of optical AGN, while hot gas accretion and one-on-one interactions are the main drivers of radio AGN activity.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

PlumX	Altmetric	Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Plumx: https://plumanalytics.com/learn/about-metrics/
Altmetric: https://www.altmetric.com/about-altmetrics/what-are-altmetrics/
Dimensions: https://www.dimensions.ai/why-dimensions/

Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

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

Colaboración Institucional

Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.

Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	ARGUDO-FERNANDEZ, MARIA DEL CARMEN	Mujer	CASSACA - China Universidad de Antofagasta - Chile Shanghai Astronomical Observatory Chinese Academy of Sciences - China
2	Shen, Shi-Yin	-	CASSACA - China Key Lab Astrophys - China Shanghai Astronomical Observatory Chinese Academy of Sciences - China Key Lab for Astrophysics - China
3	Sabater, J.	Hombre	UNIV EDINBURGH - Reino Unido University of Edinburgh, Institute for Astronomy - Reino Unido
4	Duarte Puertas, S.	-	CSIC - España Instituto de Astrofísica de Andalucía - CSIC - España
5	Verley, Simon	Hombre	UNIV GRANADA - España Universidad de Granada - España
6	Yang, X.	-	Shanghai Jiao Tong Univ - China

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Origen de Citas Identificadas

Muestra la distribución de países cuyos autores citan a la publicación consultada.

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

Citas Identificadas: 22.73 %
Citas No-identificadas: 77.27 %

Muestra la distribución de instituciones nacionales o extranjeras cuyos autores citan a la publicación consultada.

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

Citas Identificadas: 22.73 %
Citas No-identificadas: 77.27 %

Financiamiento

Fuente
National Natural Science Foundation of China
CONICYT FONDECYT
National Science Foundation
National Key Research and Development Program of China
Ministerio de Economía y Competitividad
European Regional Development Fund
Chinese Academy of Sciences
Ministerio de Economía y Competividad
National Natural Science Foundation of China (NSFC)
973 Program
Chinese Academy of Sciences (CAS)
Alfred P. Sloan Foundation
National Basic Research Program of China (973 Program)
US Department of Energy Office of Science
"Junta de Andalucia" local government
FEDER (Fondo Europeo de Desarrollo Regional)
PIFI - Chinese Academy of Sciences President's International Fellowship Initiative
Junta de Andalucia local government

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
The authors acknowledge the anonymous referee for his/her very detailed and useful report, which helped to clarify and improve the quality of this work. M.A.F. is grateful for financial support from PIFI (funded by Chinese Academy of Sciences President's International Fellowship Initiative) Grant No. 2015PM056 and from CONICYT FONDECYT project No. 3160304. This work was partly supported by the Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences (CAS; grant XDB09030200), the National Natural Science Foundation of China (NSFC) with the Project Number of 11573050 and 11433003, and the "973 Program" 2014 CB845705. This work was partially supported by Ministerio de Economia y Competividad and by FEDER (Fondo Europeo de Desarrollo Regional) via grants AYA2011-24728, AYA2013-47742-C04-01, AYA2014-53506-P, and from the "Junta de Andalucia" local government through the FQM-108 project. This research made use of ASTROPY, a community-developed core PYTHON (http://www.python.org) package for Astronomy (Astropy Collaboration et al. 2013); IPYTHON (Perez & Granger 2007); MAT-PLOTLIB (Hunter 2007); NUMPY (Walt et al. 2011); SCIPY (Jones et al. 2001); and TOPCAT (Taylor 2005). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/
This work was partly supported by the Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences (CAS; grant XDB09030200), the National Natural Science Foundation of China (NSFC) with the Project Number of 11573050 and 11433003, and the 973 Program 2014 CB845705. This work was partially supported by Ministerio de Economia y Competividad and by FEDER (Fondo Europeo de Desarrollo Regional) via grants AYA2011-24728, AYA2013-47742-C04-01, AYA2014-53506-P, and from the Junta de Andalucia local government through the FQM-108 project.

Agradecimiento

The authors acknowledge the anonymous referee for his/her very detailed and useful report, which helped to clarify and improve the quality of this work. M.A.F. is grateful for financial support from PIFI (funded by Chinese Academy of Sciences President's International Fellowship Initiative) Grant No. 2015PM056 and from CONICYT FONDECYT project No. 3160304. This work was partly supported by the Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences (CAS; grant XDB09030200), the National Natural Science Foundation of China (NSFC) with the Project Number of 11573050 and 11433003, and the "973 Program" 2014 CB845705. This work was partially supported by Ministerio de Economia y Competividad and by FEDER (Fondo Europeo de Desarrollo Regional) via grants AYA2011-24728, AYA2013-47742-C04-01, AYA2014-53506-P, and from the "Junta de Andalucia" local government through the FQM-108 project. This research made use of ASTROPY, a community-developed core PYTHON (http://www.python.org) package for Astronomy (Astropy Collaboration et al. 2013); IPYTHON (Perez & Granger 2007); MAT-PLOTLIB (Hunter 2007); NUMPY (Walt et al. 2011); SCIPY (Jones et al. 2001); and TOPCAT (Taylor 2005). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/

This work was partly supported by the Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences (CAS; grant XDB09030200), the National Natural Science Foundation of China (NSFC) with the Project Number of 11573050 and 11433003, and the 973 Program 2014 CB845705. This work was partially supported by Ministerio de Economia y Competividad and by FEDER (Fondo Europeo de Desarrollo Regional) via grants AYA2011-24728, AYA2013-47742-C04-01, AYA2014-53506-P, and from the Junta de Andalucia local government through the FQM-108 project.

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección