Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30836
Title: | Investigation of the inner structures around HD 169142 with VLT/SPHERE | Authors: | 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. |
Issue Date: | 2018 | Journal: | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | Number: | 473 | Issue: | 2 | First Page: | 1774 | 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 K<SUB>S</SUB> 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. | 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: | 0035-8711 | DOI: | 10.1093/mnras/stx2318 | Bibcode ADS: | 2018MNRAS.473.1774L | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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stx2318.pdf | PDF editoriale | 2.01 MB | Adobe PDF | View/Open |
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