Matches in SemOpenAlex for { <https://semopenalex.org/work/W2963670227> ?p ?o ?g. }
Showing items 1 to 89 of
89
with 100 items per page.
- W2963670227 endingPage "309" @default.
- W2963670227 startingPage "302" @default.
- W2963670227 abstract "Abstract A number of scenarios have been put forward to explain the origin of the chemical anomalies (and resulting complex colour-magnitude diagrams) observed in globular clusters (GCs), namely the AGB, Fast Rotating Massive Star, Very Massive Star, and Early Disc Accretion scenarios. We compare the predictions of these scenarios with a range of observations (including young massive clusters (YMCs), chemical patterns, and GC population properties) and find that all models are inconsistent with observations. In particular, YMCs do not show evidence for multiple epochs of star-formation and appear to be gas free by an age of ~ 3 Myr. Also, the chemical patterns displayed in GCs vary from one to the next in such a way that cannot be reproduced by standard nucleosynthetic yields. Finally, we show that the “mass budget problem” for the scenarios cannot be solved by invoking heavy cluster mass loss (i.e. that clusters were 10-100 times more massive at birth) as this solution makes basic predictions about the GC population that are inconsistent with observations. We conclude that none of the proposed scenarios can explain the multiple population phenomenon, hence alternative theories are needed." @default.
- W2963670227 created "2019-07-30" @default.
- W2963670227 creator A5086971577 @default.
- W2963670227 date "2015-08-01" @default.
- W2963670227 modified "2023-10-18" @default.
- W2963670227 title "A critical assessment of models for the origin of multiple populations in globular clusters" @default.
- W2963670227 cites W1646975385 @default.
- W2963670227 cites W1901877775 @default.
- W2963670227 cites W1996519895 @default.
- W2963670227 cites W2001218188 @default.
- W2963670227 cites W2016508224 @default.
- W2963670227 cites W2045692013 @default.
- W2963670227 cites W2058653821 @default.
- W2963670227 cites W2071156338 @default.
- W2963670227 cites W2073315801 @default.
- W2963670227 cites W2078314007 @default.
- W2963670227 cites W2081538426 @default.
- W2963670227 cites W2081944412 @default.
- W2963670227 cites W2088349376 @default.
- W2963670227 cites W2106695319 @default.
- W2963670227 cites W2119394279 @default.
- W2963670227 cites W2138742840 @default.
- W2963670227 cites W2142219892 @default.
- W2963670227 cites W2143775013 @default.
- W2963670227 cites W2144556453 @default.
- W2963670227 cites W2276065491 @default.
- W2963670227 cites W3099731538 @default.
- W2963670227 cites W3100090811 @default.
- W2963670227 doi "https://doi.org/10.1017/s1743921315009692" @default.
- W2963670227 hasPublicationYear "2015" @default.
- W2963670227 type Work @default.
- W2963670227 sameAs 2963670227 @default.
- W2963670227 citedByCount "1" @default.
- W2963670227 countsByYear W29636702272019 @default.
- W2963670227 crossrefType "journal-article" @default.
- W2963670227 hasAuthorship W2963670227A5086971577 @default.
- W2963670227 hasBestOaLocation W29636702271 @default.
- W2963670227 hasConcept C113461152 @default.
- W2963670227 hasConcept C121332964 @default.
- W2963670227 hasConcept C125857072 @default.
- W2963670227 hasConcept C144024400 @default.
- W2963670227 hasConcept C149923435 @default.
- W2963670227 hasConcept C150846664 @default.
- W2963670227 hasConcept C159985019 @default.
- W2963670227 hasConcept C164866538 @default.
- W2963670227 hasConcept C192562407 @default.
- W2963670227 hasConcept C199360897 @default.
- W2963670227 hasConcept C204323151 @default.
- W2963670227 hasConcept C2908647359 @default.
- W2963670227 hasConcept C41008148 @default.
- W2963670227 hasConcept C44870925 @default.
- W2963670227 hasConcept C48393594 @default.
- W2963670227 hasConceptScore W2963670227C113461152 @default.
- W2963670227 hasConceptScore W2963670227C121332964 @default.
- W2963670227 hasConceptScore W2963670227C125857072 @default.
- W2963670227 hasConceptScore W2963670227C144024400 @default.
- W2963670227 hasConceptScore W2963670227C149923435 @default.
- W2963670227 hasConceptScore W2963670227C150846664 @default.
- W2963670227 hasConceptScore W2963670227C159985019 @default.
- W2963670227 hasConceptScore W2963670227C164866538 @default.
- W2963670227 hasConceptScore W2963670227C192562407 @default.
- W2963670227 hasConceptScore W2963670227C199360897 @default.
- W2963670227 hasConceptScore W2963670227C204323151 @default.
- W2963670227 hasConceptScore W2963670227C2908647359 @default.
- W2963670227 hasConceptScore W2963670227C41008148 @default.
- W2963670227 hasConceptScore W2963670227C44870925 @default.
- W2963670227 hasConceptScore W2963670227C48393594 @default.
- W2963670227 hasIssue "S316" @default.
- W2963670227 hasLocation W29636702271 @default.
- W2963670227 hasLocation W29636702272 @default.
- W2963670227 hasOpenAccess W2963670227 @default.
- W2963670227 hasPrimaryLocation W29636702271 @default.
- W2963670227 hasRelatedWork W1590605944 @default.
- W2963670227 hasRelatedWork W1673850808 @default.
- W2963670227 hasRelatedWork W2051807879 @default.
- W2963670227 hasRelatedWork W2069375389 @default.
- W2963670227 hasRelatedWork W2138603295 @default.
- W2963670227 hasRelatedWork W2949420903 @default.
- W2963670227 hasRelatedWork W3101658532 @default.
- W2963670227 hasRelatedWork W3163083320 @default.
- W2963670227 hasRelatedWork W3211164147 @default.
- W2963670227 hasRelatedWork W4302305579 @default.
- W2963670227 hasVolume "12" @default.
- W2963670227 isParatext "false" @default.
- W2963670227 isRetracted "false" @default.
- W2963670227 magId "2963670227" @default.
- W2963670227 workType "article" @default.