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Probing the magnetospheric accretion region of the young pre-transitional disk system DoAr 44 using VLTI/GRAVITY
| Indexado |
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| DOI | 10.1051/0004-6361/202037611 | ||||
| Año | 2020 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Our results can be accounted for by a simple geometric model where the Br gamma line emission arises from a compact region interior to the inner disk edge, on a scale of a few stellar radii, fully consistent with the concept of magnetospheric accretion process in low-mass young stellar systems.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Bouvier, J. | Hombre |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 2 | Perraut, K. | Mujer |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 3 | MORALES-PERALTA, JUAN CARLOS | Hombre |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 4 | Duvert, G. | - |
Univ Grenoble Alpes - Francia
|
| 5 | Dougados, C. | Mujer |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 6 | Brandner, W. | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 7 | Benisty, Myriam | Mujer |
Univ Grenoble Alpes - Francia
Universidad de Chile - Chile Universite Grenoble Alpes - Francia |
| 8 | Berger, Jean-Philippe | Hombre |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 9 | Alecian, E. | Mujer |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| Fuente |
|---|
| European Research Council |
| European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme |
| Horizon 2020 Framework Programme |
| Agradecimiento |
|---|
| We would like to thank all the individuals who have contributed to build such a powerful instrument as GRAVITY. We thank the referees for their reports that improved the accuracy and clarity of the manuscript. This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 742095; SPIDI: Star-Planets-Inner Disk-Interactions, http://www.spidi-eu.org).This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium).Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. |
| Acknowledgements. We would like to thank all the individuals who have contributed to build such a powerful instrument as GRAVITY. We thank the referees for their reports that improved the accuracy and clarity of the manuscript. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 742095; SPIDI: Star-Planets-Inner Disk-Interactions, http://www.spidi-eu.org). This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www. cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/ consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. |
