Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29718
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Rebull, L. M. | en_US |
dc.contributor.author | Stauffer, J. R. | en_US |
dc.contributor.author | Bouvier, J. | en_US |
dc.contributor.author | Cody, A. M. | en_US |
dc.contributor.author | Hillenbrand, L. A. | en_US |
dc.contributor.author | Soderblom, D. R. | en_US |
dc.contributor.author | Valenti, J. | en_US |
dc.contributor.author | Barrado, D. | en_US |
dc.contributor.author | Bouy, H. | en_US |
dc.contributor.author | Ciardi, D. | en_US |
dc.contributor.author | Pinsonneault, M. | en_US |
dc.contributor.author | Stassun, K. | en_US |
dc.contributor.author | MICELA, Giuseppina | en_US |
dc.contributor.author | Aigrain, S. | en_US |
dc.contributor.author | Vrba, F. | en_US |
dc.contributor.author | Somers, G. | en_US |
dc.contributor.author | Gillen, E. | en_US |
dc.contributor.author | Collier Cameron, A. | en_US |
dc.date.accessioned | 2021-01-12T16:50:58Z | - |
dc.date.available | 2021-01-12T16:50:58Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29718 | - |
dc.description.abstract | We use K2 to continue the exploration of the distribution of rotation periods in Pleiades that we began in Paper I. We have discovered complicated multiperiod behavior in Pleiades stars using these K2 data, and we have grouped them into categories, which are the focal part of this paper. About 24% of the sample has multiple, real frequencies in the periodogram, sometimes manifesting as obvious beating in the LCs. Those having complex and/or structured periodogram peaks, unresolved multiple periods, and resolved close multiple periods are likely due to spot/spot group evolution and/or latitudinal differential rotation; these largely compose the slowly rotating sequence in P versus (V - K <SUB>s</SUB>)<SUB>0</SUB> identified in Paper I. The fast sequence in P versus (V - K <SUB>s</SUB>)<SUB>0</SUB> is dominated by single-period stars; these are likely to be rotating as solid bodies. Paper III continues the discussion, speculating about the origin and evolution of the period distribution in the Pleiades. | en_US |
dc.language.iso | eng | en_US |
dc.title | Rotation in the Pleiades with K2. II. Multiperiod Stars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/0004-6256/152/5/114 | en_US |
dc.identifier.scopus | 2-s2.0-84994667116 | en_US |
dc.identifier.isi | 000386139400002 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/0004-6256/152/5/114 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 152 | en_US |
dc.relation.issue | 5 | en_US |
dc.relation.firstpage | 114 | en_US |
dc.relation.numberofpages | 20 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | ESP | 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 | 2016AJ....152..114R | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | sì | 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. Palermo | - |
crisitem.author.orcid | 0000-0002-9900-4751 | - |
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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Rebull_2016_AJ_152_114.pdf | Pdf editoriale | 3.93 MB | Adobe PDF | View/Open |
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