Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34676
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Zhou, Yifan | en_US |
dc.contributor.author | Apai, Dániel | en_US |
dc.contributor.author | Lew, Ben W. P. | en_US |
dc.contributor.author | Schneider, Glenn | en_US |
dc.contributor.author | Manjavacas, Elena | en_US |
dc.contributor.author | BEDIN, Luigi | en_US |
dc.contributor.author | Cowan, Nicolas B. | en_US |
dc.contributor.author | Marley, Mark S. | en_US |
dc.contributor.author | Radigan, Jacqueline | en_US |
dc.contributor.author | Karalidi, Theodora | en_US |
dc.contributor.author | Lowrance, Patrick J. | en_US |
dc.contributor.author | Miles-Páez, Paulo A. | en_US |
dc.contributor.author | Metchev, Stanimir | en_US |
dc.contributor.author | Burgasser, Adam J. | en_US |
dc.date.accessioned | 2024-01-30T17:34:56Z | - |
dc.date.available | 2024-01-30T17:34:56Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34676 | - |
dc.description.abstract | In the third paragraph of Section 5.1, the calculated rotational breakup limit for AB Pic B omitted a factor of 2π. The rotational breakup limit of AB Pic B should correspond to a 1.57 hr rotation period instead of 0.25 hr. Therefore, the observed 2.1 hr periodic signal in AB Pic Bs light curve should be equivalent to 75% instead of 12% of the breakup limit. With a 2.1 hr rotation period and for angular momentum-conserved contraction, the rotation velocity of AB Pic B will likely approach or even exceed the breakup limit when AB Pic Bs radius approaches 1 RJup.These corrections do not affect any conclusions of the original paper. | en_US |
dc.language.iso | eng | en_US |
dc.title | Erratum: “Cloud Atlas: High-contrast Time-resolved Observations of Planetary-mass Companions” (2019, AJ, 157, 128) | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-3881/ab24dc | en_US |
dc.identifier.scopus | 2-s2.0-85072715871 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85072715871 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-3881/ab24dc | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 158 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 52 | 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 | THE ASTRONOMICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019AJ....158...52Z | 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. Padova | - |
crisitem.author.orcid | 0000-0003-4080-6466 | - |
crisitem.journal.journalissn | 0004-6256 | - |
crisitem.journal.ance | E016224 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Zhou_2019_AJ_157_128.pdf | PDF editoriale | 2.85 MB | Adobe PDF | View/Open |
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