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Investigation of the inner structures around HD 169142 with VLT/SPHERE

Ligi, R. (author)
Vigan, A. (author)
Gratton, R. (author)
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de Boer, J. (author)
Benisty, M. (author)
Boccaletti, A. (author)
Quanz, S. P. (author)
Meyer, M. (author)
Ginski, C. (author)
Sissa, E. (author)
Gry, C. (author)
Henning, T. (author)
Beuzit, J. -L. (author)
Biller, B. (author)
Bonnefoy, M. (author)
Chauvin, G. (author)
Cheetham, A. C. (author)
Cudel, M. (author)
Delorme, P. (author)
Desidera, S. (author)
Feldt, M. (author)
Galicher, R. (author)
Girard, J. (author)
Janson, Markus (author)
Stockholms universitet,Institutionen för astronomi
Kasper, M. (author)
Kopytova, T. (author)
Lagrange, A. -M. (author)
Langlois, M. (author)
Lecoroller, H. (author)
Maire, A. -L. (author)
Menard, F. (author)
Mesa, D. (author)
Peretti, S. (author)
Perrot, C. (author)
Pinilla, P. (author)
Pohl, A. (author)
Rouan, D. (author)
Stolker, T. (author)
Samland, M. (author)
Wahhaj, Z. (author)
Wildi, F. (author)
Zurlo, A. (author)
Buey, T. (author)
Fantinel, D. (author)
Fusco, T. (author)
Jaquet, M. (author)
Moulin, T. (author)
Ramos, J. (author)
Suarez, M. (author)
Weber, L. (author)
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 (creator_code:org_t)
2017-11-02
2018
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 473:2, s. 1774-1783
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We present observations of the Herbig Ae star HD 169142 with the VLT/SPHERE instruments InfraRed Dual-band Imager and Spectrograph (IRDIS) (K1K2 and H2H3 bands) and the Integral Field Spectrograph (IFS) (Y, J and H bands). We detect several bright blobs at similar to 180 mas separation from the star, and a faint arc-like structure in the IFS data. Our reference differential imaging (RDI) data analysis also finds a bright ring at the same separation. We show, using a simulation based on polarized light data, that these blobs are actually part of the ring at 180 mas. These results demonstrate that the earlier detections of blobs in the H and K-S bands at these separations in Biller et al. as potential planet/substellar companions are actually tracing a bright ring with a Keplerian motion. Moreover, we detect in the images an additional bright structure at similar to 93 mas separation and position angle of 355 degrees, at a location very close to previous detections. It appears point-like in the YJ and K bands but is more extended in the H band. We also marginally detect an inner ring in the RDI data at similar to 100 mas. Follow-up observations are necessary to confirm the detection and the nature of this source and structure.

Subject headings

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

Keyword

Stars: individual: HD169142
Planets and satellites: detection
formation
Techniques: high angular resolution
Protoplanetary disc

Publication and Content Type

ref (subject category)
art (subject category)

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