Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34329
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Renzini, Alvio | en_US |
dc.contributor.author | MARINO, Anna | en_US |
dc.contributor.author | Milone, Antonino P | en_US |
dc.date.accessioned | 2023-07-24T14:08:35Z | - |
dc.date.available | 2023-07-24T14:08:35Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34329 | - |
dc.description.abstract | Driven by recent observational findings, we select massive interactive binaries as the most suitable among the existing candidates for producing the chemical patterns typical of multiple populations of Galactic globular clusters. Still, to avoid supernova contamination we are further driven to endorse the notion that above a critical mass stars fail to produce supernova events, but rather eventually sink into black holes without ejecting much energy and heavy metals. This assumption has the attractive implication of suppressing star formation feedback for some 5--10 million years, in practice leading to runaway star formation, analog to {\it overcooling} that in absence of feedback would have turned most baryons into stars in the early Universe. Under such conditions, multiple episodes of stars formation, incorporating binary star ejecta from previous episodes, appear to be unavoidable, thus accounting for the ubiquity of the multiple population phenomenon in globular clusters. | en_US |
dc.language.iso | eng | en_US |
dc.title | The formation of globular clusters as a case of overcooling | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stac973 | en_US |
dc.identifier.scopus | 2-s2.0-85130424917 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/513/2/2111/6566354 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 513 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2111 | en_US |
dc.relation.lastpage | 2117 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | 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.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 | 0000-0002-1276-5487 | - |
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 | |
---|---|---|---|---|
stac973(1).pdf | Pdf editoriale | 435.27 kB | Adobe PDF | View/Open |
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