FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4300509218> ?p ?o ?g. }

• W4300509218 endingPage "288" @default.
• W4300509218 startingPage "279" @default.
• W4300509218 abstract "It is well appreciated that the description of overadiabatic convection affects the structure of the envelopes of luminous asymptotic giant branch (AGB) stars in the phase of “hot bottom burning” (HBB). We stress that this important uncertainty in the modeling plays a role which is much more dramatic than the role which can be ascribed, e.g., to the uncertainty in the nuclear cross-sections. Due to the role tentatively attributed today to the HBB nucleosynthesis as the site of self-enrichment of Globular Clusters stars, it is necessary to explore the difference in nucleosynthesis obtained by different prescriptions for convection. We present results of detailed evolutionary calculations of the evolution of stars of intermediate mass during the AGB phase for the metallicity typical of the Globular Clusters that show the largest spread in CNO abundances (). We follow carefully the nucleosynthesis at the base of the external convective region, showing that very different results can be obtained according to the presciption adopted to find out the temperature gradient within the instability regions. We discuss the uncertainties in the yields of the various chemical species and the role which these sources can play as polluters of the interstellar medium." @default.
• W4300509218 created "2022-10-03" @default.
• W4300509218 creator A5027465292 @default.
• W4300509218 creator A5076534405 @default.
• W4300509218 date "2005-02-01" @default.
• W4300509218 modified "2023-10-14" @default.
• W4300509218 title "Full computation of massive AGB evolution" @default.
• W4300509218 cites W1644176225 @default.
• W4300509218 cites W1968670593 @default.
• W4300509218 cites W1990218984 @default.
• W4300509218 cites W1997711174 @default.
• W4300509218 cites W2005184873 @default.
• W4300509218 cites W2011478974 @default.
• W4300509218 cites W2028925688 @default.
• W4300509218 cites W2033223848 @default.
• W4300509218 cites W2042712543 @default.
• W4300509218 cites W2048399053 @default.
• W4300509218 cites W2049561256 @default.
• W4300509218 cites W2056256517 @default.
• W4300509218 cites W2068926063 @default.
• W4300509218 cites W2073801287 @default.
• W4300509218 cites W2074687217 @default.
• W4300509218 cites W2077753988 @default.
• W4300509218 cites W2080729589 @default.
• W4300509218 cites W2088960980 @default.
• W4300509218 cites W2089699717 @default.
• W4300509218 cites W2097623445 @default.
• W4300509218 cites W2108816713 @default.
• W4300509218 cites W2119095722 @default.
• W4300509218 cites W2121463223 @default.
• W4300509218 cites W2165266750 @default.
• W4300509218 cites W2952828037 @default.
• W4300509218 cites W3022214567 @default.
• W4300509218 cites W3098130767 @default.
• W4300509218 cites W3098705288 @default.
• W4300509218 cites W3099819036 @default.
• W4300509218 cites W3100302987 @default.
• W4300509218 cites W3101010933 @default.
• W4300509218 cites W3102379822 @default.
• W4300509218 cites W3103447097 @default.
• W4300509218 cites W34215931 @default.
• W4300509218 cites W4299584246 @default.
• W4300509218 doi "https://doi.org/10.1051/0004-6361:20041917" @default.
• W4300509218 hasPublicationYear "2005" @default.
• W4300509218 type Work @default.
• W4300509218 citedByCount "159" @default.
• W4300509218 countsByYear W43005092182012 @default.
• W4300509218 countsByYear W43005092182013 @default.
• W4300509218 countsByYear W43005092182014 @default.
• W4300509218 countsByYear W43005092182015 @default.
• W4300509218 countsByYear W43005092182016 @default.
• W4300509218 countsByYear W43005092182017 @default.
• W4300509218 countsByYear W43005092182018 @default.
• W4300509218 countsByYear W43005092182019 @default.
• W4300509218 countsByYear W43005092182020 @default.
• W4300509218 countsByYear W43005092182021 @default.
• W4300509218 countsByYear W43005092182022 @default.
• W4300509218 countsByYear W43005092182023 @default.
• W4300509218 crossrefType "journal-article" @default.
• W4300509218 hasAuthorship W4300509218A5027465292 @default.
• W4300509218 hasAuthorship W4300509218A5076534405 @default.
• W4300509218 hasBestOaLocation W43005092181 @default.
• W4300509218 hasConcept C10899652 @default.
• W4300509218 hasConcept C110472602 @default.
• W4300509218 hasConcept C112473583 @default.
• W4300509218 hasConcept C113461152 @default.
• W4300509218 hasConcept C121332964 @default.
• W4300509218 hasConcept C1276947 @default.
• W4300509218 hasConcept C150846664 @default.
• W4300509218 hasConcept C181313176 @default.
• W4300509218 hasConcept C4397270 @default.
• W4300509218 hasConcept C44870925 @default.
• W4300509218 hasConcept C97355855 @default.
• W4300509218 hasConcept C99465377 @default.
• W4300509218 hasConceptScore W4300509218C10899652 @default.
• W4300509218 hasConceptScore W4300509218C110472602 @default.
• W4300509218 hasConceptScore W4300509218C112473583 @default.
• W4300509218 hasConceptScore W4300509218C113461152 @default.
• W4300509218 hasConceptScore W4300509218C121332964 @default.
• W4300509218 hasConceptScore W4300509218C1276947 @default.
• W4300509218 hasConceptScore W4300509218C150846664 @default.
• W4300509218 hasConceptScore W4300509218C181313176 @default.
• W4300509218 hasConceptScore W4300509218C4397270 @default.
• W4300509218 hasConceptScore W4300509218C44870925 @default.
• W4300509218 hasConceptScore W4300509218C97355855 @default.
• W4300509218 hasConceptScore W4300509218C99465377 @default.
• W4300509218 hasIssue "1" @default.
• W4300509218 hasLocation W43005092181 @default.
• W4300509218 hasLocation W43005092182 @default.
• W4300509218 hasLocation W43005092183 @default.
• W4300509218 hasOpenAccess W4300509218 @default.
• W4300509218 hasPrimaryLocation W43005092181 @default.
• W4300509218 hasRelatedWork W2013531135 @default.
• W4300509218 hasRelatedWork W2081379755 @default.
• W4300509218 hasRelatedWork W2089507342 @default.
• W4300509218 hasRelatedWork W2141691962 @default.
• W4300509218 hasRelatedWork W2141818940 @default.
• W4300509218 hasRelatedWork W3104777999 @default.

• next