FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2055261854> ?p ?o ?g. }

• W2055261854 endingPage "944" @default.
• W2055261854 startingPage "937" @default.
• W2055261854 abstract "<i>Context. <i/>Atomic diffusion is believed to be an important physical process in the atmospheres of several types of stars. Stellar atmospheres, including the stratification of the elements due to diffusion, are then needed to properly compare theoretical results to observations for such stars.<i>Aims. <i/>This paper aims to estimate the effect of vertical abundance stratification on the atmospheric structure of stars and its potential importance regarding observational anomalies for various types of stars.<i>Methods. <i/>Simulations using a modified version of the PHOENIX atmosphere code will be described, while taking vertical abundance stratification into account.<i>Results. <i/>Our results show that large abundance gradients can exist in the atmospheres of Ap and blue horizontal branch stars. Stratification can also lead to relatively large atmospheric structural changes. The effect of elemental stratification on the atmospheric structure might well be able to explain the well-known core-wing anomaly of the Balmer lines observed for cool Ap stars." @default.
• W2055261854 created "2016-06-24" @default.
• W2055261854 creator A5003970599 @default.
• W2055261854 creator A5014273433 @default.
• W2055261854 creator A5057058925 @default.
• W2055261854 creator A5087141427 @default.
• W2055261854 date "2009-01-14" @default.
• W2055261854 modified "2023-09-30" @default.
• W2055261854 title "Stellar model atmospheres with abundance stratification" @default.
• W2055261854 cites W1548323710 @default.
• W2055261854 cites W1611556424 @default.
• W2055261854 cites W164385788 @default.
• W2055261854 cites W1710938835 @default.
• W2055261854 cites W1981923898 @default.
• W2055261854 cites W1982717132 @default.
• W2055261854 cites W1988136156 @default.
• W2055261854 cites W1994058135 @default.
• W2055261854 cites W2011415806 @default.
• W2055261854 cites W2019744752 @default.
• W2055261854 cites W2057089807 @default.
• W2055261854 cites W2059211296 @default.
• W2055261854 cites W2077557604 @default.
• W2055261854 cites W2090434735 @default.
• W2055261854 cites W2092682287 @default.
• W2055261854 cites W2103524055 @default.
• W2055261854 cites W2108193003 @default.
• W2055261854 cites W2114918372 @default.
• W2055261854 cites W2132635528 @default.
• W2055261854 cites W2141487670 @default.
• W2055261854 cites W2147053842 @default.
• W2055261854 cites W2149577635 @default.
• W2055261854 cites W3098576339 @default.
• W2055261854 cites W3098799628 @default.
• W2055261854 cites W3099134501 @default.
• W2055261854 cites W3099993199 @default.
• W2055261854 cites W3101390372 @default.
• W2055261854 cites W4289256463 @default.
• W2055261854 cites W4292406868 @default.
• W2055261854 cites W4299352420 @default.
• W2055261854 doi "https://doi.org/10.1051/0004-6361:200810848" @default.
• W2055261854 hasPublicationYear "2009" @default.
• W2055261854 type Work @default.
• W2055261854 sameAs 2055261854 @default.
• W2055261854 citedByCount "81" @default.
• W2055261854 countsByYear W20552618542012 @default.
• W2055261854 countsByYear W20552618542013 @default.
• W2055261854 countsByYear W20552618542014 @default.
• W2055261854 countsByYear W20552618542015 @default.
• W2055261854 countsByYear W20552618542016 @default.
• W2055261854 countsByYear W20552618542017 @default.
• W2055261854 countsByYear W20552618542018 @default.
• W2055261854 countsByYear W20552618542019 @default.
• W2055261854 countsByYear W20552618542020 @default.
• W2055261854 countsByYear W20552618542021 @default.
• W2055261854 countsByYear W20552618542022 @default.
• W2055261854 countsByYear W20552618542023 @default.
• W2055261854 crossrefType "journal-article" @default.
• W2055261854 hasAuthorship W2055261854A5003970599 @default.
• W2055261854 hasAuthorship W2055261854A5014273433 @default.
• W2055261854 hasAuthorship W2055261854A5057058925 @default.
• W2055261854 hasAuthorship W2055261854A5087141427 @default.
• W2055261854 hasBestOaLocation W20552618541 @default.
• W2055261854 hasConcept C100701293 @default.
• W2055261854 hasConcept C101638190 @default.
• W2055261854 hasConcept C121332964 @default.
• W2055261854 hasConcept C150846664 @default.
• W2055261854 hasConcept C153294291 @default.
• W2055261854 hasConcept C192943249 @default.
• W2055261854 hasConcept C3527866 @default.
• W2055261854 hasConcept C44870925 @default.
• W2055261854 hasConcept C59822182 @default.
• W2055261854 hasConcept C62279395 @default.
• W2055261854 hasConcept C65440619 @default.
• W2055261854 hasConcept C86803240 @default.
• W2055261854 hasConcept C88548481 @default.
• W2055261854 hasConceptScore W2055261854C100701293 @default.
• W2055261854 hasConceptScore W2055261854C101638190 @default.
• W2055261854 hasConceptScore W2055261854C121332964 @default.
• W2055261854 hasConceptScore W2055261854C150846664 @default.
• W2055261854 hasConceptScore W2055261854C153294291 @default.
• W2055261854 hasConceptScore W2055261854C192943249 @default.
• W2055261854 hasConceptScore W2055261854C3527866 @default.
• W2055261854 hasConceptScore W2055261854C44870925 @default.
• W2055261854 hasConceptScore W2055261854C59822182 @default.
• W2055261854 hasConceptScore W2055261854C62279395 @default.
• W2055261854 hasConceptScore W2055261854C65440619 @default.
• W2055261854 hasConceptScore W2055261854C86803240 @default.
• W2055261854 hasConceptScore W2055261854C88548481 @default.
• W2055261854 hasIssue "3" @default.
• W2055261854 hasLocation W20552618541 @default.
• W2055261854 hasLocation W20552618542 @default.
• W2055261854 hasLocation W20552618543 @default.
• W2055261854 hasLocation W20552618544 @default.
• W2055261854 hasOpenAccess W2055261854 @default.
• W2055261854 hasPrimaryLocation W20552618541 @default.
• W2055261854 hasRelatedWork W1593053234 @default.
• W2055261854 hasRelatedWork W1986109513 @default.
• W2055261854 hasRelatedWork W2028449984 @default.

• next