Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/33004
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Fontanive, C. | en_US |
dc.contributor.author | BEDIN, Luigi | en_US |
dc.contributor.author | Bardalez Gagliuffi, D. C. | en_US |
dc.date.accessioned | 2023-01-23T15:38:35Z | - |
dc.date.available | 2023-01-23T15:38:35Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33004 | - |
dc.description.abstract | In this paper, we present our project that aims at determining accurate distances and proper motions for the Y brown dwarf population using the Hubble Space Telescope. We validate the program with our first results, using a single new epoch of observations of the Y0pec dwarf WISE J163940.83-684738.6. These new data allowed us to refine its proper motion and improve the accuracy of its parallax by a factor of three compared to previous determinations, now constrained to ϖ = 211.11 ± 0.56 mas. This newly derived absolute parallax corresponds to a distance of 4.737 ± 0.013 pc, an exquisite and unprecedented precision for faint ultracool Y dwarfs. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Y dwarf population with HST: unlocking the secrets of our coolest neighbours - I. Overview and first astrometric results | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/staa3732 | en_US |
dc.identifier.scopus | 2-s2.0-85100386344 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/501/1/911/6017306 | en_US |
dc.identifier.url | http://arxiv.org/abs/2011.13873v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 501 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 911 | en_US |
dc.relation.lastpage | 915 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | 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 | 2021MNRAS.501..911F | 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.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0003-4080-6466 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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staa3732.pdf | Pdf editoriale | 333.99 kB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.