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Discovery of a point-like source and a third spiral arm in the transition disk around the Herbig Ae star MWC 758

Reggiani, M (author)
Université de Liège, Belgium
Christiaens, V (author)
Université de Liège, Belgium
Absil, O (author)
Université de Liège, Belgium
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Mawet, D (author)
California Institute of Technology, USA
Huby, E (author)
Observatoire de Paris, Sorbonne Universités, France
Choquet, E (author)
Jet Propulsion Laboratory, USA
Gomez Gonzalez, C.A. (author)
Université de Liège, Belgium
Ruane, G (author)
California Institute of Technology, USA
Femenia, B (author)
W. M. Keck Observatory, USA
Serabyn, E (author)
Jet Propulsion Laboratory, USA
Matthews, K (author)
California Institute of Technology, USA
Barraza, M (author)
Universidad de Chile, Chile
Carlomagno, B (author)
Université de Liège, Belgium
Defrère, D (author)
Université de Liège, Belgium
Delacroix, C (author)
Université de Liège, Belgium
Habraken, S (author)
Université de Liège, Belgium
Jolivet, A (author)
Université de Liège, Belgium
Karlsson, Mikael (author)
Uppsala universitet,Tillämpad materialvetenskap
Orban de Xivry, G (author)
Université de Liège, Belgium
Piron, Pierre (author)
Uppsala universitet,Tillämpad materialvetenskap
Surdej, J (author)
Université de Liège, Belgium
Vargas Catalan, Ernesto, 1988- (author)
Uppsala universitet,Tillämpad materialvetenskap
Wertz, O (author)
Argelander-Institut für Astronomie, Germany
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 (creator_code:org_t)
2018-03-29
2018
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 611
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Context. Transition disks offer the extraordinary opportunity to look for newly born planets and to investigate the early stages of planet formation. Aims. In this context we observed the Herbig A5 star MWC 758 with the L'-band vector vortex coronagraph installed in the near-infrared camera and spectrograph NIRC2 at the Keck II telescope, with the aim of unveiling the nature of the spiral structure by constraining the presence of planetary companions in the system. Methods. Our high-contrast imaging observations show a bright (Delta L' = 7.0 +/- 0.3 mag) point-like emission south of MWC 758 at a deprojected separation of similar to 20 au (r = 0 ''.111 +/- 0 ''.004) from the central star. We also recover the two spiral arms (southeast and northwest), already imaged by previous studies in polarized light, and discover a third arm to the southwest of the star. No additional companions were detected in the system down to 5 Jupiter masses beyond 0 ''.6 from the star. Results. We propose that the bright L'-band emission could be caused by the presence of an embedded and accreting protoplanet, although the possibility of it being an asymmetric disk feature cannot be excluded. The spiral structure is probably not related to the protoplanet candidate, unless on an inclined and eccentric orbit, and it could be due to one (or more) yet undetected planetary companions at the edge of or outside the spiral pattern. Future observations and additional simulations will be needed to shed light on the true nature of the point-like source and its link with the spiral arms.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

protoplanetary disks
planet-disk interactions
stars: pre-main sequence
stars: individual: MWC 758 (HD 36112)

Publication and Content Type

ref (subject category)
art (subject category)

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