Dataciencia

Colección SciELO Chile

Ruling out unresolved binaries in five transitional disks VLT/NACO deep 2.12 and 1.75 mu m narrow-band imaging

Indexado

WoS	WOS:000295168100135
Scopus	SCOPUS_ID:80052875229

DOI

10.1051/0004-6361/201016294

Año

2011

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. These new VLT/NACO observations further constrain the origin of the inner opacity cavities to be owing to closer or lower- mass companions or other mechanisms such as giant planet formation, efficient grain growth, and photoevaporation (for DoAr 21 and HR 4796A).

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	Vicente, Sílvia	Mujer	European Space Agcy ESTEC - Países Bajos ESTEC - European Space Research and Technology Centre - Países Bajos
2	Merin, B.	Hombre	European Space Agcy ESAC - España European Space Astronomy Centre - España European Space Agcy ESTEC - España
3	Hartung, Markus	Hombre	AURA Chile - Chile Gemini ObservatorySouthern Operations Center - Chile
4	Bouy, H.	Hombre	LAEFF - España Centro de Astrobiología (CSIC-INTA) - España
5	Huelamo, Nuria	Mujer	LAEFF - España Centro de Astrobiología (CSIC-INTA) - España
6	Artigau, Étienne	Hombre	UNIV MONTREAL - Canadá University of Montreal - Canadá
7	Augereau, Jean-Charles	Hombre	UJF Grenoble 1 CNRS INSU - Francia Verimag - Francia Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
8	van Dishoeck, E. F.	-	Leiden Univ - Países Bajos Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos
9	Olofsson, Johan	Hombre	Max Planck Inst Astron - Alemania Max Planck Institute for Astronomy - Alemania
10	Oliveira, Isa	-	Leiden Univ - Países Bajos Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos
11	Prusti, T.	Hombre	European Space Agcy ESTEC - Países Bajos ESTEC - European Space Research and Technology Centre - Países Bajos

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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: 38.46 %
Citas No-identificadas: 61.54 %

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

Citas Identificadas: 38.46 %
Citas No-identificadas: 61.54 %

Financiamiento

Fuente
National Science Foundation
National Aeronautics and Space Administration
Association of Canadian Universities for Research in Astronomy
ESA Science Faculty
Association of Universities for Research in Astronomy Inc.

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
The authors thank the anonymous referee for important comments, which improved this paper, and to Catia Cardoso for fruitful discussion on binary dynamics. Support in the preparation of this publication was provided by the ESA Science Faculty. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of the Vizier Service provided by the Centre de Donnees Astronomiques de Strasbourg, France (Ochsenbein et al. 2000). Image Reduction and Analysis Facility (IRAF) is distributed by the National Optical Astronomy Observatory (NOAO), which is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under cooperative agreement with the National Science Foundation (NSF).
The authors thank the anonymous referee for important comments, which improved this paper, and to Cátia Cardoso for fruitful discussion on binary dynamics. Support in the preparation of this publication was provided by the ESA Science Faculty. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of the Vizier Service provided by the Centre de Données Astronomiques de Strasbourg, France (Ochsenbein et al. 2000). Image Reduction and Analysis Facility (IRAF) is distributed by the National Optical Astronomy Observatory (NOAO), which is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under cooperative agreement with the National Science Foundation (NSF).

Agradecimiento

The authors thank the anonymous referee for important comments, which improved this paper, and to Catia Cardoso for fruitful discussion on binary dynamics. Support in the preparation of this publication was provided by the ESA Science Faculty. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of the Vizier Service provided by the Centre de Donnees Astronomiques de Strasbourg, France (Ochsenbein et al. 2000). Image Reduction and Analysis Facility (IRAF) is distributed by the National Optical Astronomy Observatory (NOAO), which is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under cooperative agreement with the National Science Foundation (NSF).

The authors thank the anonymous referee for important comments, which improved this paper, and to Cátia Cardoso for fruitful discussion on binary dynamics. Support in the preparation of this publication was provided by the ESA Science Faculty. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of the Vizier Service provided by the Centre de Données Astronomiques de Strasbourg, France (Ochsenbein et al. 2000). Image Reduction and Analysis Facility (IRAF) is distributed by the National Optical Astronomy Observatory (NOAO), which is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under cooperative agreement with the National Science Foundation (NSF).

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