Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26232
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Cabrera-Ziri, I. | en_US |
dc.contributor.author | Niederhofer, F. | en_US |
dc.contributor.author | Bastian, N. | en_US |
dc.contributor.author | Rejkuba, M. | en_US |
dc.contributor.author | Balbinot, E. | en_US |
dc.contributor.author | Kerzendorf, W. E. | en_US |
dc.contributor.author | Larsen, S. S. | en_US |
dc.contributor.author | Mackey, A. D. | en_US |
dc.contributor.author | Dalessandro, Emanuele | en_US |
dc.contributor.author | Mucciarelli, A. | en_US |
dc.contributor.author | Charbonnel, C. | en_US |
dc.contributor.author | Hilker, M. | en_US |
dc.contributor.author | Gieles, M. | en_US |
dc.contributor.author | Hénault-Brunet, V. | en_US |
dc.date.accessioned | 2020-06-26T12:34:54Z | - |
dc.date.available | 2020-06-26T12:34:54Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26232 | - |
dc.description.abstract | Recently, Li et al. claimed to have found evidence for multiple generations of stars in the intermediate-age clusters NGC 1783, NGC 1806 and NGC 411 in the Large and Small Magellanic Clouds. Here we show that these young stellar populations are present in the field regions around these clusters and are not likely associated with the clusters themselves. Using the same data sets, we find that the background subtraction method adopted by the authors does not adequately remove contaminating stars in the small number Poisson limit. Hence, we conclude that their results do not provide evidence of young generations of stars within these clusters. | en_US |
dc.language.iso | eng | en_US |
dc.title | No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw966 | en_US |
dc.identifier.scopus | 2-s2.0-84979253675 | en_US |
dc.identifier.isi | 000379830700062 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/459/4/4218/2624074 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 459 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 4218 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | NLD | en_US |
dc.contributor.country | CHE | 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 | 2016MNRAS.459.4218C | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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 | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-4237-4601 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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stw966.pdf | Pdf editoriale | 25.35 MB | Adobe PDF | View/Open |
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