Matches in SemOpenAlex for { <https://semopenalex.org/work/W2891024622> ?p ?o ?g. }
- W2891024622 endingPage "8" @default.
- W2891024622 startingPage "8" @default.
- W2891024622 abstract "Motivated by the desire to measure beryllium abundances in red giant stars, we have constructed a new line list for synthesizing spectra in the near-ultraviolet. Using the Sun, Arcturus, and Pollux as benchmark stars, we explore potential sources of missing continuous opacity and line absorption. Despite the inclusion of new sources of continuous opacity, fitting the ultraviolet OH lines in the solar spectrum still requires artificially inflating the continuous opacity. The red giants also require the addition of a line of unknown origin in the blue wing of the Be line at λ3131.065 Å, and we find a good match can be made by adopting a Ti ii line with low excitation potential. The inclusion of this line does not affect the measurement of the solar Be abundance. Because the fits to all of the benchmark stars require tuning the properties of known spectral lines and including both an unknown source of additional continuous opacity and spectral lines of unknown origin, we argue that the absolute abundances of Be in stars should be interpreted with caution. Therefore, the question of whether the solar Be abundance is depleted may not yet be resolved, although our model favors minimal Be depletion in the Sun." @default.
- W2891024622 created "2018-09-27" @default.
- W2891024622 creator A5004357483 @default.
- W2891024622 creator A5005195344 @default.
- W2891024622 creator A5007265287 @default.
- W2891024622 creator A5059358944 @default.
- W2891024622 date "2018-09-17" @default.
- W2891024622 modified "2023-09-27" @default.
- W2891024622 title "An Updated Line List for NUV Spectral Synthesis in Evolved Stars: Redetermination of the Beryllium Abundance in the Solar Photosphere" @default.
- W2891024622 cites W1534858351 @default.
- W2891024622 cites W1659875532 @default.
- W2891024622 cites W1672426287 @default.
- W2891024622 cites W1927791180 @default.
- W2891024622 cites W1964585777 @default.
- W2891024622 cites W1977457396 @default.
- W2891024622 cites W1982940613 @default.
- W2891024622 cites W2011493866 @default.
- W2891024622 cites W2013285605 @default.
- W2891024622 cites W2014586054 @default.
- W2891024622 cites W2022231983 @default.
- W2891024622 cites W2025881578 @default.
- W2891024622 cites W2026914150 @default.
- W2891024622 cites W2029384527 @default.
- W2891024622 cites W2038540839 @default.
- W2891024622 cites W2048872220 @default.
- W2891024622 cites W2054959040 @default.
- W2891024622 cites W2057951961 @default.
- W2891024622 cites W2060089153 @default.
- W2891024622 cites W2085358324 @default.
- W2891024622 cites W2096471541 @default.
- W2891024622 cites W2104302410 @default.
- W2891024622 cites W2110679917 @default.
- W2891024622 cites W2123829915 @default.
- W2891024622 cites W2126741668 @default.
- W2891024622 cites W2132358681 @default.
- W2891024622 cites W2132963711 @default.
- W2891024622 cites W2136109064 @default.
- W2891024622 cites W2155908710 @default.
- W2891024622 cites W2161866432 @default.
- W2891024622 cites W2165593927 @default.
- W2891024622 cites W2254725139 @default.
- W2891024622 cites W2297676747 @default.
- W2891024622 cites W2602055580 @default.
- W2891024622 cites W2899497983 @default.
- W2891024622 cites W3099218389 @default.
- W2891024622 cites W3100530444 @default.
- W2891024622 cites W3102855917 @default.
- W2891024622 cites W3105803879 @default.
- W2891024622 cites W4290960035 @default.
- W2891024622 cites W4292399985 @default.
- W2891024622 cites W4298427325 @default.
- W2891024622 doi "https://doi.org/10.3847/1538-4357/aad8bf" @default.
- W2891024622 hasPublicationYear "2018" @default.
- W2891024622 type Work @default.
- W2891024622 sameAs 2891024622 @default.
- W2891024622 citedByCount "4" @default.
- W2891024622 countsByYear W28910246222019 @default.
- W2891024622 countsByYear W28910246222020 @default.
- W2891024622 countsByYear W28910246222022 @default.
- W2891024622 crossrefType "journal-article" @default.
- W2891024622 hasAuthorship W2891024622A5004357483 @default.
- W2891024622 hasAuthorship W2891024622A5005195344 @default.
- W2891024622 hasAuthorship W2891024622A5007265287 @default.
- W2891024622 hasAuthorship W2891024622A5059358944 @default.
- W2891024622 hasBestOaLocation W28910246221 @default.
- W2891024622 hasConcept C108884401 @default.
- W2891024622 hasConcept C121332964 @default.
- W2891024622 hasConcept C1276947 @default.
- W2891024622 hasConcept C150846664 @default.
- W2891024622 hasConcept C185544564 @default.
- W2891024622 hasConcept C198352243 @default.
- W2891024622 hasConcept C2524010 @default.
- W2891024622 hasConcept C33923547 @default.
- W2891024622 hasConcept C44870925 @default.
- W2891024622 hasConcept C4839761 @default.
- W2891024622 hasConcept C505870484 @default.
- W2891024622 hasConcept C506630978 @default.
- W2891024622 hasConcept C77077793 @default.
- W2891024622 hasConcept C86803240 @default.
- W2891024622 hasConceptScore W2891024622C108884401 @default.
- W2891024622 hasConceptScore W2891024622C121332964 @default.
- W2891024622 hasConceptScore W2891024622C1276947 @default.
- W2891024622 hasConceptScore W2891024622C150846664 @default.
- W2891024622 hasConceptScore W2891024622C185544564 @default.
- W2891024622 hasConceptScore W2891024622C198352243 @default.
- W2891024622 hasConceptScore W2891024622C2524010 @default.
- W2891024622 hasConceptScore W2891024622C33923547 @default.
- W2891024622 hasConceptScore W2891024622C44870925 @default.
- W2891024622 hasConceptScore W2891024622C4839761 @default.
- W2891024622 hasConceptScore W2891024622C505870484 @default.
- W2891024622 hasConceptScore W2891024622C506630978 @default.
- W2891024622 hasConceptScore W2891024622C77077793 @default.
- W2891024622 hasConceptScore W2891024622C86803240 @default.
- W2891024622 hasIssue "1" @default.
- W2891024622 hasLocation W28910246221 @default.
- W2891024622 hasLocation W28910246222 @default.
- W2891024622 hasOpenAccess W2891024622 @default.
- W2891024622 hasPrimaryLocation W28910246221 @default.