Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30836
DC Field | Value | Language |
---|---|---|
dc.contributor.author | LIGI, ROXANNE | en_US |
dc.contributor.author | Vigan, A. | en_US |
dc.contributor.author | GRATTON, Raffaele | en_US |
dc.contributor.author | de Boer, J. | en_US |
dc.contributor.author | Benisty, M. | en_US |
dc.contributor.author | Boccaletti, A. | en_US |
dc.contributor.author | Quanz, S. P. | en_US |
dc.contributor.author | Meyer, M. | en_US |
dc.contributor.author | Ginski, C. | en_US |
dc.contributor.author | Sissa, E. | en_US |
dc.contributor.author | Gry, C. | en_US |
dc.contributor.author | Henning, T. | en_US |
dc.contributor.author | Beuzit, J. -L. | en_US |
dc.contributor.author | Biller, B. | en_US |
dc.contributor.author | Bonnefoy, M. | en_US |
dc.contributor.author | Chauvin, G. | en_US |
dc.contributor.author | Cheetham, A. C. | en_US |
dc.contributor.author | Cudel, M. | en_US |
dc.contributor.author | Delorme, P. | en_US |
dc.contributor.author | DESIDERA, Silvano | en_US |
dc.contributor.author | Feldt, M. | en_US |
dc.contributor.author | Galicher, R. | en_US |
dc.contributor.author | Girard, J. | en_US |
dc.contributor.author | Janson, M. | en_US |
dc.contributor.author | Kasper, M. | en_US |
dc.contributor.author | Kopytova, T. | en_US |
dc.contributor.author | Lagrange, A. -M. | en_US |
dc.contributor.author | Langlois, M. | en_US |
dc.contributor.author | Lecoroller, H. | en_US |
dc.contributor.author | Maire, A. -L. | en_US |
dc.contributor.author | Ménard, F. | en_US |
dc.contributor.author | MESA, DINO | en_US |
dc.contributor.author | Peretti, S. | en_US |
dc.contributor.author | Perrot, C. | en_US |
dc.contributor.author | Pinilla, P. | en_US |
dc.contributor.author | Pohl, A. | en_US |
dc.contributor.author | Rouan, D. | en_US |
dc.contributor.author | Stolker, T. | en_US |
dc.contributor.author | Samland, M. | en_US |
dc.contributor.author | Wahhaj, Z. | en_US |
dc.contributor.author | Wildi, F. | en_US |
dc.contributor.author | Zurlo, A. | en_US |
dc.contributor.author | Buey, T. | en_US |
dc.contributor.author | FANTINEL, Daniela | en_US |
dc.contributor.author | Fusco, T. | en_US |
dc.contributor.author | Jaquet, M. | en_US |
dc.contributor.author | Moulin, T. | en_US |
dc.contributor.author | Ramos, J. | en_US |
dc.contributor.author | Suarez, M. | en_US |
dc.contributor.author | Weber, L. | en_US |
dc.date.accessioned | 2021-04-21T15:01:41Z | - |
dc.date.available | 2021-04-21T15:01:41Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30836 | - |
dc.description.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. | en_US |
dc.language.iso | eng | en_US |
dc.title | Investigation of the inner structures around HD 169142 with VLT/SPHERE | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx2318 | en_US |
dc.identifier.scopus | 2-s2.0-85038909013 | en_US |
dc.identifier.url | http://arxiv.org/abs/1709.01734v2 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/473/2/1774/4587911 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 473 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 1774 | en_US |
dc.relation.lastpage | 1783 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018MNRAS.473.1774L | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-6257-6051 | - |
crisitem.author.orcid | 0000-0003-2195-6805 | - |
crisitem.author.orcid | 0000-0001-8613-2589 | - |
crisitem.author.orcid | 0000-0001-8467-1933 | - |
crisitem.author.orcid | 0000-0001-8152-9480 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
---|---|---|---|---|
stx2318.pdf | PDF editoriale | 2.01 MB | Adobe PDF | View/Open |
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