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| Indexado |
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| DOI | 10.1051/0004-6361/202038337 | ||||
| Año | 2020 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. Based on the morphology analysis, we favor the scenario that assumes the scattered light is coming from a circumstellar disk rather than the outflow around EX Lup. We determine the origin of the observed feature as either coming from a continuous circumstellar disk with a cavity, from the illuminated wall of the outer disk, or from a shadowed disk. Moreover, we discuss the potential origins of the depleted region of mu m-size grains, exploring the possibility that a sub-stellar companion may be the source of this feature.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Rigliaco, E. | - |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 2 | Gratton, Raffaele | Hombre |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 3 | Kóspál, Ágnes | Mujer |
Res Ctr Astron & Earth Sci - Hungría
Max Planck Inst Astron - Alemania Eotvos Lorand Univ - Hungría Konkoly Observatory - Hungría Max Planck Institute for Astronomy - Alemania Eötvös Loránd University - Hungría Eötvös Loránd Tudományegyetem - Hungría |
| 4 | Mesa, Dino | Hombre |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 5 | D'Orazi, Valentina | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 6 | Abraham, P. | Hombre |
Res Ctr Astron & Earth Sci - Hungría
Eotvos Lorand Univ - Hungría Konkoly Observatory - Hungría Eötvös Loránd University - Hungría Eötvös Loránd Tudományegyetem - Hungría |
| 7 | Desidera, S. | Hombre |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 8 | Ginski, Ch. | Hombre |
Univ Amsterdam - Países Bajos
Leiden Univ - Países Bajos Universiteit van Amsterdam - Países Bajos Leiden Observatory Research Institute - Países Bajos Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos Sterrewacht Leiden - Países Bajos |
| 9 | van Holstein, R. G. | Hombre |
Leiden Univ - Países Bajos
ESO - Chile Leiden Observatory Research Institute - Países Bajos European Southern Observatory Santiago - Chile Sterrewacht Leiden - Países Bajos European Southern Observ - Chile |
| 10 | Dominik, C. | Hombre |
Univ Amsterdam - Países Bajos
Universiteit van Amsterdam - Países Bajos Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos |
| 11 | Garufi, A. | Hombre |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astrofisico Di Arcetri - Italia INAF - Italia |
| 12 | Henning, Thomas | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 13 | Menard, Francois | Hombre |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 14 | Zurlo, Alice | Mujer |
Universidad Diego Portales - Chile
Aix Marseille Univ - Francia Laboratoire d'Astrophysique de Marseille - Francia |
| 15 | Baruffolo, A. | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia INAF - Italia |
| 16 | Maurel, D. | - |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 17 | COSTA-DUARTE, M., V | Mujer |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 18 | Weber, Luc | - |
Univ Geneva - Suiza
Université de Genève - Suiza Faculty of Science - Suiza |
| Fuente |
|---|
| European Commission |
| European Research Council |
| ESO |
| Seventh Framework Programme |
| CNRS (France) |
| MPIA (Germany) |
| INAF (Italy) |
| FINES (Switzerland) |
| NOVA (Netherlands) |
| ASI-INAF |
| Ministero dell’Istruzione, dell’Università e della Ricerca |
| European Research Council (ERC) under the European Union |
| H2020 Marie Skłodowska-Curie Actions |
| Horizon 2020 |
| Centre National de la Recherche Scientifique |
| Horizon 2020 Framework Programme |
| MPIA |
| Istituto Nazionale di Astrofisica |
| Italian Ministry of Education, University |
| FINES |
| European Commission Sixth and Seventh Framework Programmes |
| Nova |
| Nederlandse Onderzoekschool voor Astronomie |
| European Research Council under the Horizon 2020 Framework Program via the ERC |
| Italian Ministry of Education, University, and Research |
| Max-Planck-Institut fur Astronomie |
| project PRIN INAF 2016 The Cradle of Life - GENESIS-SKA (General Conditions in Early Planetary Systems for the rise of life with SKA) |
| European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant |
| Agradecimiento |
|---|
| E.R. is supported by the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 664931. E.R. and S.D. acknowledge financial support from the ASI-INAF agreement n.2018-16-HH.0. This work has been supported by the project PRIN INAF 2016 The Cradle of Life - GENESIS-SKA (General Conditions in Early Planetary Systems for the rise of life with SKA) and by the "Progetti Premiali" funding scheme of the Italian Ministry of Education, University, and Research. This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme under grant agreement No 716155. T.H. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Advanced Grant Origins 83 24 28. SPHERE is an instrument designed and built by a consortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF Osservatorio Astronomico di Padova (Italy), Observatoire de Geneve (Switzerland), ETH Zurich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Framework Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 (2004-2008), grant number 226604 for FP7 (2009-2012), and grant number 312430 for FP7 (2013-2016). |
| cA knolw edgemens. E.R. is supported by the European Unions Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 664931. E.R. and S.D. acknowledge financial support from the ASI-INAF agreement n.2018-16-HH.0. This work has been supported by the project PRIN INAF 2016 The Cradle of Life – GENESIS-SKA (General Conditions in Early Planetary Systems for the rise of life with SKA) and by the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 716155. T.H. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Advanced Grant Origins 83 24 28. SPHERE is an instrument designed and built by a consortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF Osservatorio Astronomico di Padova (Italy), Observatoire de Geneve (Switzerland), ETH Zurich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Framework Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 (2004-2008), grant number 226604 for FP7 (2009-2012), and grant number 312430 for FP7 (2013-2016). |