Dataciencia

Colección SciELO Chile

Differential interferometric phases at high spectral resolution as a sensitive physical diagnostic of circumstellar disks

Indexado

WoS	WOS:000322008600076
Scopus	SCOPUS_ID:84879771009

DOI

10.1051/0004-6361/201321313

Año

2013

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The full power of this diagnostic tool can be expected if it can be applied to observations over a full life-cycle of a disk from first ejection through final dispersal, over a full cycle of disk oscillations, or over a full orbital period in a binary system.

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	Faes, Daniel M.	Hombre	UNIV SAO PAULO - Brasil Univ Nice Sophia Antipolis - Francia Universidade de Sao Paulo - USP - Brasil Laboratoire Joseph-Louis Lagrange - Francia Universidade de São Paulo - Brasil
2	Carciofi, A. C.	-	UNIV SAO PAULO - Brasil
3	Rivinius, Th	Hombre	Observatorio Europeo Austral - Chile European Organisation for Astronomical Research in the Southern Hemisphere - Chile
4	Stefl, S.	-	Atacama Large Millimeter Array - Chile
5	Baade, D.	Hombre	ESO - Alemania European Organisation for Astronomical Research in the Southern Hemisphere - Alemania Observatorio Europeo Austral - Chile European Organisation for Astronomical Research in the Southern Hemisphere - Chile
6	de Souza, A. Domiciano	-	Univ Nice Sophia Antipolis - Francia
6	Domiciano De Souza, A.	-	Laboratoire Joseph-Louis Lagrange - Francia Univ Nice Sophia Antipolis - Francia

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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: 33.33 %
Citas No-identificadas: 66.67 %

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

Citas Identificadas: 33.33 %
Citas No-identificadas: 66.67 %

Financiamiento

Fuente
CNPq
FAPESP
Fundação de Amparo à Pesquisa do Estado de São Paulo
FundaÃ§Ã£o de Amparo Ã Pesquisa do Estado de SÃ£o Paulo
CNRS-PICS
Brazilian agency FAPESP

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Agradecimientos

Agradecimiento
D.M.F., A. C. C. and A. D. S. thank the CNRS-PICS program for supporting our Brazilian-French collaboration and the present work. D. M. F. acknowledges support from FAPESP (grant 2012/04916-7). A. C. C. acknowledges support from CNPq (grant 307076/2012-1) and FAPESP (grant 2010/19029-0). This work has made use of the computing facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by the Brazilian agency FAPESP (grant 2009/54006-4) and the INCT-A.
D.M.F., A.C.C. and A.D.S. thank the CNRS-PICS program for supporting our Brazilian-French collaboration and the present work. D.M.F. acknowledges support from FAPESP (grant 2012/04916-7). A.C.C. acknowledges support from CNPq (grant 307076/2012-1) and FAPESP (grant 2010/19029-0). This work has made use of the computing facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by the Brazilian agency FAPESP (grant 2009/54006-4) and the INCT-A.

Agradecimiento

D.M.F., A. C. C. and A. D. S. thank the CNRS-PICS program for supporting our Brazilian-French collaboration and the present work. D. M. F. acknowledges support from FAPESP (grant 2012/04916-7). A. C. C. acknowledges support from CNPq (grant 307076/2012-1) and FAPESP (grant 2010/19029-0). This work has made use of the computing facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by the Brazilian agency FAPESP (grant 2009/54006-4) and the INCT-A.

D.M.F., A.C.C. and A.D.S. thank the CNRS-PICS program for supporting our Brazilian-French collaboration and the present work. D.M.F. acknowledges support from FAPESP (grant 2012/04916-7). A.C.C. acknowledges support from CNPq (grant 307076/2012-1) and FAPESP (grant 2010/19029-0). This work has made use of the computing facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by the Brazilian agency FAPESP (grant 2009/54006-4) and the INCT-A.