Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26717
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BRAGAGLIA, Angela | en_US |
dc.date.accessioned | 2020-08-19T10:29:18Z | - |
dc.date.available | 2020-08-19T10:29:18Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1743-9213 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26717 | - |
dc.description.abstract | The contribution of massive star clusters to their hosting halo dramatically depends on their formation mechanism and their early evolution. Massive globular clusters in the Milky Way (and in other galaxies) have been shown to display peculiar chemical patterns (light-elements correlations and anti-correlations) indicative of a complex star formation, confirmed by photometric evidence (spread or split sequences). I use these chemical signatures to try to understand what is the fraction of halo stars originally born in globular clusters. | en_US |
dc.language.iso | eng | en_US |
dc.title | Contribution of globular clusters to halos | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1017/S1743921315009138 | en_US |
dc.identifier.scopus | 2-s2.0-85016590826 | en_US |
dc.identifier.isi | 000456237800069 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/contribution-of-globular-clusters-to-halos/F8CDFE8E7A15CC508D2F14D38FFB393D | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | vol. 12, S316 | en_US |
dc.relation.firstpage | 287 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.ispartofbook | Formation, Evolution, and Survival of Massive Star Clusters | en_US |
dc.type.invited | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | en_US |
dc.identifier.adsbibcode | 2017IAUS..316..287B | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-0338-7883 | - |
crisitem.journal.journalissn | 1743-9213 | - |
crisitem.journal.ance | E192651 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
contribution_of_globular_clusters_to_halos.pdf | PDF editoriale | 2.05 MB | Adobe PDF | View/Open |
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