Dataciencia

Colección SciELO Chile

Molecular gas content and SFR in Hickson compact groups: enhanced or deficient?

Indexado

WoS	WOS:000303315400110
Scopus	SCOPUS_ID:84859311493

DOI

10.1051/0004-6361/201117281

Año

2012

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The properties of M-H2 and L-FIR in galaxies in HCGs are surprisingly similar to those of isolated galaxies, in spite of the much higher Def(M-HI) of the former. The trends of the sSFR and Def(M-H2) with Def(M-HI) and the evolutionary state indicate, however, that the ongoing interaction might have some effect on the molecular gas and SF.

Revista

Revista	ISSN
Astronomy & Astrophysics	1432-0746

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	Martinez-Badenes, V.	-	CSIC - España Instituto de Astrofísica de Andalucía - CSIC - España
2	Lisenfeld, Ute	-	UNIV GRANADA - España Universidad de Granada, Facultad de Ciencias - España
3	Espada, Daniel	Hombre	CSIC - España Natl Astron Observ Japan - Japón Instituto de Astrofísica de Andalucía - CSIC - España National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
4	Verdes-Montenegro, Lourdes	Mujer	CSIC - España Instituto de Astrofísica de Andalucía - CSIC - España
5	Garcia-Burillo, S.	Hombre	Observ Madrid - España Observatorio Astronomico Nacional - España
6	Leon, Stephane	-	Atacama Large Millimeter Array - Chile
7	Sulentic, J.	Hombre	CSIC - España Instituto de Astrofísica de Andalucía - CSIC - España
8	Yun, Min	Mujer	Univ Massachusetts - Estados Unidos University of Massachusetts Amherst - Estados Unidos

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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: 11.11 %
Citas No-identificadas: 88.89 %

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

Citas Identificadas: 11.11 %
Citas No-identificadas: 88.89 %

Financiamiento

Fuente
National Science Foundation
Junta de Andalucía
NSF
European Community
National Aeronautics and Space Administration
Junta de Andalucia (Spain)
Junta de AndalucÃa
Ministerio de Ciencia TecnologÃa y Telecomunicaciones
Spanish Ministerio de Ciencia y Educacion
6th European Community Framework Program
Directorate for Mathematical and Physical Sciences
Ministerio de Educación Superior, Ciencia y Tecnología, República Dominicana

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
This work has been supported by the research projects AYA2008-06181-C02 and AYA2007-67625-C02-02 from the Spanish Ministerio de Ciencia y Educacion and the Junta de Andalucia (Spain) grants P08-FQM-4205, FQM-0108 and TIC-114. D. E. was supported by a Marie Curie International Fellowship within the 6th European Community Framework Program (MOIF-CT-2006-40298). U. L. warmly thanks IPAC (Caltech) for their hospitality during a sabbatical stay when this work was finished. We also thank T. Bitsakis and V. Charmandaris for letting us use their Spitzer data prior to publication, and the anonymous referee for critical comments that helped to put our conclusions on a firmer ground and improved the quality of the paper. This work is based on observations with the Instituto de Radioastronomia Milimetrica IRAM 30 m and the Five College Radio Astronomy (FCRAO) 14 m. The FCRAO is supported by NSF grant AST 0838222. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We also acknowledge the usage of the HyperLeda database (http://leda.univ-lyon1.fr).
This work has been supported by the research projects AYA2008-06181-C02 and AYA2007-67625-C02-02 from the Spanish Ministerio de Ciencia y Educación and the Junta de Andalucía (Spain) grants P08-FQM-4205, FQM-0108 and TIC-114. D.E. was supported by a Marie Curie International Fellowship within the 6th European Community Framework Program (MOIF-CT-2006-40298). U.L. warmly thanks IPAC (Caltech) for their hospitality during a sabbatical stay when this work was finished. We also thank T. Bitsakis and V. Charmandaris for letting us use their Spitzer data prior to publication, and the anonymous referee for critical comments that helped to put our conclusions on a firmer ground and improved the quality of the paper. This work is based on observations with the Instituto de Radioastronomia Milimétrica IRAM 30 m and the Five College Radio Astronomy (FCRAO) 14 m. The FCRAO is supported by NSF grant AST 0838222. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We also acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ).

Agradecimiento

This work has been supported by the research projects AYA2008-06181-C02 and AYA2007-67625-C02-02 from the Spanish Ministerio de Ciencia y Educacion and the Junta de Andalucia (Spain) grants P08-FQM-4205, FQM-0108 and TIC-114. D. E. was supported by a Marie Curie International Fellowship within the 6th European Community Framework Program (MOIF-CT-2006-40298). U. L. warmly thanks IPAC (Caltech) for their hospitality during a sabbatical stay when this work was finished. We also thank T. Bitsakis and V. Charmandaris for letting us use their Spitzer data prior to publication, and the anonymous referee for critical comments that helped to put our conclusions on a firmer ground and improved the quality of the paper. This work is based on observations with the Instituto de Radioastronomia Milimetrica IRAM 30 m and the Five College Radio Astronomy (FCRAO) 14 m. The FCRAO is supported by NSF grant AST 0838222. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We also acknowledge the usage of the HyperLeda database (http://leda.univ-lyon1.fr).

This work has been supported by the research projects AYA2008-06181-C02 and AYA2007-67625-C02-02 from the Spanish Ministerio de Ciencia y Educación and the Junta de Andalucía (Spain) grants P08-FQM-4205, FQM-0108 and TIC-114. D.E. was supported by a Marie Curie International Fellowship within the 6th European Community Framework Program (MOIF-CT-2006-40298). U.L. warmly thanks IPAC (Caltech) for their hospitality during a sabbatical stay when this work was finished. We also thank T. Bitsakis and V. Charmandaris for letting us use their Spitzer data prior to publication, and the anonymous referee for critical comments that helped to put our conclusions on a firmer ground and improved the quality of the paper. This work is based on observations with the Instituto de Radioastronomia Milimétrica IRAM 30 m and the Five College Radio Astronomy (FCRAO) 14 m. The FCRAO is supported by NSF grant AST 0838222. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We also acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ).

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