Rings and gaps in the disc around Elias 24 revealed by ALMA
Author
dc.contributor.author
Dipierro, G.
Author
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Ricci, L.
Author
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Pérez Muñoz, Laura
Author
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Lodato, G.
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Alexander, R. D.
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Laibe, G.
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Andrews, S.
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Carpenter, J. M.
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Chandler, C. J.
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Greaves, J. A.
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Hall, C.
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Henning, Thomas
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Kwon, W.
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Linz, H.
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Mundy, L.
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Sargent, A.
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Tazzari, M.
Author
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Testi, L.
Author
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Wilner, D.
Admission date
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2018-07-20T19:38:14Z
Available date
dc.date.available
2018-07-20T19:38:14Z
Publication date
dc.date.issued
2018
Cita de ítem
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Monthly Notices of The Royal Astronomical Society 475, 5296-5321 (2018)
es_ES
Identifier
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10.1093/mnras/sty181
Identifier
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https://repositorio.uchile.cl/handle/2250/150102
Abstract
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We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle 2 observations of the 1.3-mm dust continuum emission of the protoplanetary disc surrounding the T Tauri star Elias 24 with an angular resolution of similar to 0.2 arcsec (similar to 28 au). The dust continuum emission map reveals a dark ring at a radial distance of 0.47 arcsec (similar to 65 au) from the central star, surrounded by a bright ring at 0.58 arcsec (similar to 81 au). In the outer disc, the radial intensity profile shows two inflection points at 0.71 and 0.87 arcsec (similar to 99 and 121 au, respectively). We perform global three-dimensional smoothed particle hydrodynamic gas/dust simulations of discs hosting a migrating and accreting planet. Combining the dust density maps of small and large grains with three-dimensional radiative transfer calculations, we produce synthetic ALMA observations of a variety of disc models in order to reproduce the gap-and ring-like features observed in Elias 24. We find that the dust emission across the disc is consistent with the presence of an embedded planet with a mass of similar to 0.7 M-J at an orbital radius of similar to 60 au. Our model suggests that the two inflection points in the radial intensity profile are due to the inward radial motion of large dust grains from the outer disc. The surface brightness map of our disc model provides a reasonable match to the gap-and ring-like structures observed in Elias 24, with an average discrepancy of similar to 5 per cent of the observed fluxes around the gap region.
es_ES
Patrocinador
dc.description.sponsorship
CIERA postdoctoral fellowship at Northwestern University
NASA Fermi
NNX15AU69G
NASA
NNX12AG44G
NSF
1412144