Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/24342
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | MASSARI, DAVIDE | en_US |
dc.contributor.author | Lapenna, Emilio | en_US |
dc.contributor.author | BRAGAGLIA, Angela | en_US |
dc.contributor.author | Dalessandro, Emanuele | en_US |
dc.contributor.author | Contreras Ramos, Rodrigo | en_US |
dc.contributor.author | Amigo, Pía | en_US |
dc.date.accessioned | 2020-04-29T16:03:48Z | - |
dc.date.available | 2020-04-29T16:03:48Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24342 | - |
dc.description.abstract | We present Strömgren photometry of the Galactic Globular Cluster M3 to study its multiple generations phenomenon. The use of different colour-magnitude diagrams (CMDs) and especially of the notoriously efficient c<SUB>y</SUB> index allowed us to detect a double red giant branch in the cluster CMD. After decontamination from fore- and background sources, the two sequences turned out to be equally populated. The two components also show a bimodal radial distribution well corresponding to that predicted by numerical simulations for clusters living in an intermediate dynamical evolutive state and with a population with modified chemical composition that was born more centrally concentrated than the primordial. The analysis of high-resolution spectra quantitatively demonstrates that the two detected sequences correspond to the first (Na-poor) generation and the second (Na-rich) generation, thus confirming the importance of synergy between photometry and spectroscopy. | en_US |
dc.language.iso | eng | en_US |
dc.title | Multiple stellar populations in the globular cluster M3 (NGC 5272): a Strömgren perspective | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw583 | en_US |
dc.identifier.scopus | 2-s2.0-84965002020 | en_US |
dc.identifier.isi | 000375799500061 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/458/4/4162/2613855 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 458 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 4162 | 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 | 2016MNRAS.458.4162M | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò 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.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-0338-7883 | - |
crisitem.author.orcid | 0000-0003-4237-4601 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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172_massari_stromgren_m3_2016.pdf | pdf editoriale | 7.54 MB | Adobe PDF | Visualizza/apri |
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