Dataciencia

Colección SciELO Chile

The binary Be star δ Scorpii at high spectral and spatial resolution : I. Disk geometry and kinematics before the 2011 periastron

Indexado

WoS	WOS:000293283600091
Scopus	SCOPUS_ID:79960794490

DOI

10.1051/0004-6361/201116798

Año

2011

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. As the star probably rotates at about 70% of its critical velocity, the ejection of matter does not seem to be dominated by rotation. However, the disk geometry and kinematics are similar to the previously studied quasi-critically rotating Be stars, alpha Ara, psi Per and 48 Per.

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	Meilland, Anthony	Hombre	Max Planck Inst Radioastron - Alemania Max Planck Institute for Radio Astronomy - Alemania
2	Delaa, O.	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
3	Stee, P.	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
4	Kanaan, Samer	Hombre	Universidad de Valparaíso - Chile
5	Millour, Florentin	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
6	Mourard, D.	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
7	Bonneau, D.	-	CNRS - Francia Observatoire de la Côte d'Azur - Francia
8	Petrov, Romain	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
9	Nardetto, N.	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
10	Marcotto, Aurelie	Mujer	CNRS - Francia Observatoire de la Côte d'Azur - Francia
11	Roussel, A.	-	CNRS - Francia Observatoire de la Côte d'Azur - Francia
12	Clausse, Jean-Michel	Hombre	CNRS - Francia Observatoire de la Côte d'Azur - Francia
13	Perraut, K.	Mujer	UJF CNRS LAOG - Francia Universite Grenoble Alpes - Francia
14	Mc Alister, Harold A.	Hombre	Georgia State Univ - Estados Unidos Mt Wilson Observ - Estados Unidos Georgia State University - Estados Unidos Mount Wilson Observatory - Estados Unidos
15	ten Brummelaar, Theo	Hombre	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - Estados Unidos
16	Sturmann, Judit	Mujer	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - Estados Unidos
17	Sturmann, Laszlo	-	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - Estados Unidos
18	Turner, Neal	Hombre	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - Estados Unidos
19	Ridgway, Stephen T.	Hombre	Natl Opt Astron Observ - Estados Unidos National Optical Astronomy Observatory - Estados Unidos
20	Farrington, Christopher D.	Hombre	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - Estados Unidos
21	Goldfinger, P. J.	-	Mt Wilson Observ - Estados Unidos Mount Wilson Observatory - 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: 18.75 %
Citas No-identificadas: 81.25 %

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

Citas Identificadas: 18.75 %
Citas No-identificadas: 81.25 %

Financiamiento

Fuente
National Science Foundation
NASA
National Aeronautics and Space Administration
W. M. Keck Foundation
NASA Exoplanet Science Institute
INSU
PACA
CanceropÃ´le PACA
VedeckÃ¡ GrantovÃ¡ AgentÃºra MÅ VVaÅ SR a SAV
Gemini-CONICYT
Georgia State University
Region PACA
French program ASHRA
French program PNPS
Max Planck Institut fur Radioastronomy
CHARA
Vedecká Grantová Agentúra MŠVVaŠ SR a SAV
Directorate for Mathematical and Physical Sciences

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
A. Meilland acknowledges financial support from the Max Planck Institut fur Radioastronomy. VEGA is a collaboration between CHARA and OCA/LAOG/CRAL/LESIA that has been supported by the French programs PNPS and ASHRA, by INSU, and by the Region PACA. The project has obviously benefitted from strong support of the OCA and CHARA technical teams. The CHARA Array is operated with support from the National Science Foundation through grant AST-0908253, the W. M. Keck Foundation, the NASA Exoplanet Science Institute, and from Georgia State University. This work has made use of the BeSS database, operated at GEPI, Observatoire de Meudon, France: http://basebe.obspm.fr, use of the Jean-Marie Mariotti Center SearchCal service<SUP>5</SUP> co-developed by FIZEAU and LAOG, and of CDS Astronomical Databases SIMBAD and VIZIER<SUP>6</SUP>. This work has also made use of the Jean-Marie Mariotti Center LITpro service co-developed by CRAL, LAOG, and FIZEAU<SUP>7</SUP>. S.T.R. acknowledges partial support from NASA grant NNH09AK731. S. Kanaan acknowledges financial support from the GEMINI-CONICYT Fund, allocated to the project No. 32090006.
A. Meilland acknowledges financial support from the Max Planck Institut für Radioastronomy. VEGA is a collaboration between CHARA and OCA/LAOG/CRAL/LESIA that has been supported by the French programs PNPS and ASHRA, by INSU, and by the Région PACA. The project has obviously benefitted from strong support of the OCA and CHARA technical teams. The CHARA Array is operated with support from the National Science Foundation through grant AST-0908253, the W. M. Keck Foundation, the NASA Exoplanet Science Institute, and from Georgia State University. This work has made use of the BeSS database, operated at GEPI, Observatoire de Meudon, France: http://basebe.obspm.fr , use of the Jean-Marie Mariotti Center SearchCal service5 co-developed by FIZEAU and LAOG, and of CDS Astronomical Databases SIMBAD and VIZIER6.This work has also made use of the Jean-Marie Mariotti Center LITpro service co-developed by CRAL, LAOG, and FIZEAU7. S.T.R. acknowledges partial support from NASA grant NNH09AK731. S. Kanaan acknowledges financial support from the GEMINI-CONICYT Fund, allocated to the project No. 32090006.

Agradecimiento

A. Meilland acknowledges financial support from the Max Planck Institut fur Radioastronomy. VEGA is a collaboration between CHARA and OCA/LAOG/CRAL/LESIA that has been supported by the French programs PNPS and ASHRA, by INSU, and by the Region PACA. The project has obviously benefitted from strong support of the OCA and CHARA technical teams. The CHARA Array is operated with support from the National Science Foundation through grant AST-0908253, the W. M. Keck Foundation, the NASA Exoplanet Science Institute, and from Georgia State University. This work has made use of the BeSS database, operated at GEPI, Observatoire de Meudon, France: http://basebe.obspm.fr, use of the Jean-Marie Mariotti Center SearchCal service5 co-developed by FIZEAU and LAOG, and of CDS Astronomical Databases SIMBAD and VIZIER6. This work has also made use of the Jean-Marie Mariotti Center LITpro service co-developed by CRAL, LAOG, and FIZEAU7. S.T.R. acknowledges partial support from NASA grant NNH09AK731. S. Kanaan acknowledges financial support from the GEMINI-CONICYT Fund, allocated to the project No. 32090006.

A. Meilland acknowledges financial support from the Max Planck Institut für Radioastronomy. VEGA is a collaboration between CHARA and OCA/LAOG/CRAL/LESIA that has been supported by the French programs PNPS and ASHRA, by INSU, and by the Région PACA. The project has obviously benefitted from strong support of the OCA and CHARA technical teams. The CHARA Array is operated with support from the National Science Foundation through grant AST-0908253, the W. M. Keck Foundation, the NASA Exoplanet Science Institute, and from Georgia State University. This work has made use of the BeSS database, operated at GEPI, Observatoire de Meudon, France: http://basebe.obspm.fr , use of the Jean-Marie Mariotti Center SearchCal service5 co-developed by FIZEAU and LAOG, and of CDS Astronomical Databases SIMBAD and VIZIER6.This work has also made use of the Jean-Marie Mariotti Center LITpro service co-developed by CRAL, LAOG, and FIZEAU7. S.T.R. acknowledges partial support from NASA grant NNH09AK731. S. Kanaan acknowledges financial support from the GEMINI-CONICYT Fund, allocated to the project No. 32090006.

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