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

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

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2018
Author(s)
LIGI, ROXANNE  
•
Vigan, A.
•
GRATTON, Raffaele  
•
de Boer, J.
•
Benisty, M.
•
Boccaletti, A.
•
Quanz, S. P.
•
Meyer, M.
•
Ginski, C.
•
Sissa, E.
•
Gry, C.
•
Henning, T.
•
Beuzit, J. -L.
•
Biller, B.
•
Bonnefoy, M.
•
Chauvin, G.
•
Cheetham, A. C.
•
Cudel, M.
•
Delorme, P.
•
DESIDERA, Silvano  
•
Feldt, M.
•
Galicher, R.
•
Girard, J.
•
Janson, M.
•
Kasper, M.
•
Kopytova, T.
•
Lagrange, A. -M.
•
Langlois, M.
•
Lecoroller, H.
•
Maire, A. -L.
•
Ménard, F.
•
MESA, DINO  
•
Peretti, S.
•
Perrot, C.
•
Pinilla, P.
•
Pohl, A.
•
Rouan, D.
•
Stolker, T.
•
Samland, M.
•
Wahhaj, Z.
•
Wildi, F.
•
Zurlo, A.
•
Buey, T.
•
FANTINEL, Daniela  
•
Fusco, T.
•
Jaquet, M.
•
Moulin, T.
•
Ramos, J.
•
Suarez, M.
•
Weber, L.
DOI
10.1093/mnras/stx2318
Abstract
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 ˜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 KS 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 ˜93 mas separation and position angle of 355°, 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 ˜100 mas. Follow-up observations are necessary to confirm the detection and the nature of this source and structure.
Volume
473
Issue
2
Start page
1774
Uri
http://hdl.handle.net/20.500.12386/30836
Url
http://arxiv.org/abs/1709.01734v2
https://academic.oup.com/mnras/article/473/2/1774/4587911
Issn Identifier
0035-8711
Ads BibCode
2018MNRAS.473.1774L
Rights
open.access
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