Dataciencia

Colección SciELO Chile

Deconstructing the Antlia cluster core

Indexado

WoS	WOS:000366936800124
Scopus	SCOPUS_ID:84948947486

DOI

10.1051/0004-6361/201527136

Año

2015

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The high radial velocity dispersion of galaxies in the Antlia region reflects a considerable extension along the line of sight.

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	Caso, Juan P.	Hombre	UNIV NACL LA PLATA - Argentina UNLP - Argentina Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina Universidad Nacional de La Plata - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
2	Richtler, T.	-	Universidad de Concepción - Chile

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

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: 16.67 %
Citas No-identificadas: 83.33 %

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

Citas Identificadas: 16.67 %
Citas No-identificadas: 83.33 %

Financiamiento

Fuente
FONDECYT
Agencia Nacional de Promoción Científica y Tecnológica
Universidad Nacional de La Plata
National Science Foundation
Comisión Nacional de Investigación Científica y Tecnológica
Australian Research Council
Ministerio de Ciencia, Tecnología e Innovación Productiva
National Research Council
Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina
ComisiÃ³n Nacional de InvestigaciÃ³n CientÃfica y TecnolÃ³gica
Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica
ESO Telescopes at the La Silla Paranal Observatory
BASAL Centro de Astrofisica y Tecnologias Afines (CATA)
Ministerio da Ciencia, Tecnologia e Inovacao
Fondo Nacional de Desarrollo CientÃfico, TecnolÃ³gico y de InnovaciÃ³n TecnolÃ³gica
Agencia Nacional de PromociÃ³n CientÃfica y TecnolÃ³gica
Ministerio de Ciencia, TecnologÃa e InnovaciÃ³n Productiva
MinistÃ©rio da CiÃªncia, Tecnologia e InovaÃ§Ã£o
Universidad Nacional de La Plata (Argentina)

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
We thank Ylva Schuberth for discussions about the radial velocities of Virgo galaxies, Mike Fellhauer for permission to use his orbit program, Francisco Azpillicueta for discussions of statistical issues, and Lilia Bassino for discussions about the Antlia cluster. We thank the refereee for suggestions that improved this article. This work was based on observations made with ESO telescopes at the La Silla Paranal Observatory under programmes ID 60.A-905 and ID 079.B-0480, and on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministerio da Ciencia, Tecnologia e Inovacao (Brazil) and Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina), and on observations acquired through the Gemini Science Archive. 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. This work was funded with grants from Consejo Nacional de Investigaciones Cientificas y Tecnicas de la Republica Argentina, Agencia Nacional de Promocion Cientifica y Tecnologica (BID AR PICT-2013-0317), and Universidad Nacional de La Plata (Argentina). T.R. is grateful for financial support from FONDECYT project Nr. 1100620, and from the BASAL Centro de Astrofisica y Tecnologias Afines (CATA) PFB-06/2007.
We thank Ylva Schuberth for discussions about the radial velocities of Virgo galaxies, Mike Fellhauer for permission to use his orbit program, Francisco Azpillicueta for discussions of statistical issues, and Lilia Bassino for discussions about the Antlia cluster. We thank the refereee for suggestions that improved this article. This work was based on observations made with ESO telescopes at the La Silla Paranal Observatory under programmes ID 60.A-905 and ID 079.B-0480, and on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and on observations acquired through the Gemini Science Archive. 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. This work was funded with grants from Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina, Agencia Nacional de Promoción Científica y Tecnológica (BID AR PICT-2013-0317), and Universidad Nacional de La Plata (Argentina). T.R. is grateful for financial support from FONDECYT project Nr. 1100620, and from the BASAL Centro de Astrofísica y Tecnologías Afines (CATA) PFB-06/2007.

Agradecimiento

We thank Ylva Schuberth for discussions about the radial velocities of Virgo galaxies, Mike Fellhauer for permission to use his orbit program, Francisco Azpillicueta for discussions of statistical issues, and Lilia Bassino for discussions about the Antlia cluster. We thank the refereee for suggestions that improved this article. This work was based on observations made with ESO telescopes at the La Silla Paranal Observatory under programmes ID 60.A-905 and ID 079.B-0480, and on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministerio da Ciencia, Tecnologia e Inovacao (Brazil) and Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina), and on observations acquired through the Gemini Science Archive. 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. This work was funded with grants from Consejo Nacional de Investigaciones Cientificas y Tecnicas de la Republica Argentina, Agencia Nacional de Promocion Cientifica y Tecnologica (BID AR PICT-2013-0317), and Universidad Nacional de La Plata (Argentina). T.R. is grateful for financial support from FONDECYT project Nr. 1100620, and from the BASAL Centro de Astrofisica y Tecnologias Afines (CATA) PFB-06/2007.

We thank Ylva Schuberth for discussions about the radial velocities of Virgo galaxies, Mike Fellhauer for permission to use his orbit program, Francisco Azpillicueta for discussions of statistical issues, and Lilia Bassino for discussions about the Antlia cluster. We thank the refereee for suggestions that improved this article. This work was based on observations made with ESO telescopes at the La Silla Paranal Observatory under programmes ID 60.A-905 and ID 079.B-0480, and on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and on observations acquired through the Gemini Science Archive. 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. This work was funded with grants from Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina, Agencia Nacional de Promoción Científica y Tecnológica (BID AR PICT-2013-0317), and Universidad Nacional de La Plata (Argentina). T.R. is grateful for financial support from FONDECYT project Nr. 1100620, and from the BASAL Centro de Astrofísica y Tecnologías Afines (CATA) PFB-06/2007.

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