FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3121740744> ?p ?o ?g. }

• W3121740744 endingPage "69" @default.
• W3121740744 startingPage "69" @default.
• W3121740744 abstract "The Lyman-alpha emission line dominates the far-ultraviolet spectra of late-type stars and is a major source for photodissociation of important molecules including H2O, CH4, and CO2 in exoplanet atmospheres. The incident flux in this line illuminating an exoplanet's atmosphere cannot be measured directly as neutral hydrogen in the interstellar medium (ISM) attenuates most of the flux reaching the Earth. Reconstruction of the intrinsic Lyman-alpha line has been accomplished for a limited number of nearby stars, but is not feasible for distant or faint host stars. We identify correlations connecting the intrinsic Lyman-alpha flux with the flux in other emission lines formed in the stellar chromosphere, and find that these correlations depend only gradually on the flux in the other lines. These correlations, which are based on HST spectra, reconstructed Lyman-alpha line fluxes, and irradiance spectra of the quiet and active Sun, are required for photochemical models of exoplanet atmospheres when intrinsic Lyman-alpha fluxes are not available. We find a tight correlation of the intrinsic Lyman-alpha flux with stellar X-ray flux for F5 V to K5 V stars, but much larger dispersion for M stars. We also show that knowledge of the stellar effective temperature and rotation rate can provide reasonably accurate estimates of the Lyman-alpha flux for G and K stars, and less accurate estimates for cooler stars." @default.
• W3121740744 created "2021-02-01" @default.
• W3121740744 creator A5026684651 @default.
• W3121740744 creator A5083165380 @default.
• W3121740744 date "2013-03-08" @default.
• W3121740744 modified "2023-10-14" @default.
• W3121740744 title "COMPUTING INTRINSIC LYα FLUXES OF F5 V TO M5 V STARS" @default.
• W3121740744 cites W1819610785 @default.
• W3121740744 cites W1967267230 @default.
• W3121740744 cites W1975825441 @default.
• W3121740744 cites W1979760653 @default.
• W3121740744 cites W1980383716 @default.
• W3121740744 cites W1988500538 @default.
• W3121740744 cites W1990134539 @default.
• W3121740744 cites W1998069062 @default.
• W3121740744 cites W2008790307 @default.
• W3121740744 cites W2012056991 @default.
• W3121740744 cites W2026052621 @default.
• W3121740744 cites W2027645770 @default.
• W3121740744 cites W2031959188 @default.
• W3121740744 cites W2032802648 @default.
• W3121740744 cites W2037170534 @default.
• W3121740744 cites W2044183576 @default.
• W3121740744 cites W2045984796 @default.
• W3121740744 cites W2054959040 @default.
• W3121740744 cites W2059577626 @default.
• W3121740744 cites W2073891539 @default.
• W3121740744 cites W2082329580 @default.
• W3121740744 cites W2083745993 @default.
• W3121740744 cites W2084695302 @default.
• W3121740744 cites W2102812128 @default.
• W3121740744 cites W2107833438 @default.
• W3121740744 cites W2117323971 @default.
• W3121740744 cites W2143171135 @default.
• W3121740744 cites W2161459806 @default.
• W3121740744 cites W2741326455 @default.
• W3121740744 cites W2762265283 @default.
• W3121740744 cites W3020842808 @default.
• W3121740744 cites W3100275256 @default.
• W3121740744 cites W3100702394 @default.
• W3121740744 cites W3100933089 @default.
• W3121740744 cites W3101452792 @default.
• W3121740744 cites W3103985000 @default.
• W3121740744 cites W3104572572 @default.
• W3121740744 cites W3104646949 @default.
• W3121740744 cites W4240970399 @default.
• W3121740744 cites W4291818094 @default.
• W3121740744 cites W4293676342 @default.
• W3121740744 doi "https://doi.org/10.1088/0004-637x/766/2/69" @default.
• W3121740744 hasPublicationYear "2013" @default.
• W3121740744 type Work @default.
• W3121740744 sameAs 3121740744 @default.
• W3121740744 citedByCount "96" @default.
• W3121740744 countsByYear W31217407442012 @default.
• W3121740744 countsByYear W31217407442013 @default.
• W3121740744 countsByYear W31217407442014 @default.
• W3121740744 countsByYear W31217407442015 @default.
• W3121740744 countsByYear W31217407442016 @default.
• W3121740744 countsByYear W31217407442017 @default.
• W3121740744 countsByYear W31217407442018 @default.
• W3121740744 countsByYear W31217407442019 @default.
• W3121740744 countsByYear W31217407442020 @default.
• W3121740744 countsByYear W31217407442021 @default.
• W3121740744 countsByYear W31217407442022 @default.
• W3121740744 countsByYear W31217407442023 @default.
• W3121740744 crossrefType "journal-article" @default.
• W3121740744 hasAuthorship W3121740744A5026684651 @default.
• W3121740744 hasAuthorship W3121740744A5083165380 @default.
• W3121740744 hasBestOaLocation W31217407441 @default.
• W3121740744 hasConcept C101638190 @default.
• W3121740744 hasConcept C121332964 @default.
• W3121740744 hasConcept C1276947 @default.
• W3121740744 hasConcept C150846664 @default.
• W3121740744 hasConcept C163479331 @default.
• W3121740744 hasConcept C191897082 @default.
• W3121740744 hasConcept C192562407 @default.
• W3121740744 hasConcept C196939603 @default.
• W3121740744 hasConcept C198352243 @default.
• W3121740744 hasConcept C2524010 @default.
• W3121740744 hasConcept C33923547 @default.
• W3121740744 hasConcept C44870925 @default.
• W3121740744 hasConcept C4839761 @default.
• W3121740744 hasConcept C68709404 @default.
• W3121740744 hasConcept C98444146 @default.
• W3121740744 hasConcept C99465377 @default.
• W3121740744 hasConceptScore W3121740744C101638190 @default.
• W3121740744 hasConceptScore W3121740744C121332964 @default.
• W3121740744 hasConceptScore W3121740744C1276947 @default.
• W3121740744 hasConceptScore W3121740744C150846664 @default.
• W3121740744 hasConceptScore W3121740744C163479331 @default.
• W3121740744 hasConceptScore W3121740744C191897082 @default.
• W3121740744 hasConceptScore W3121740744C192562407 @default.
• W3121740744 hasConceptScore W3121740744C196939603 @default.
• W3121740744 hasConceptScore W3121740744C198352243 @default.
• W3121740744 hasConceptScore W3121740744C2524010 @default.
• W3121740744 hasConceptScore W3121740744C33923547 @default.
• W3121740744 hasConceptScore W3121740744C44870925 @default.
• W3121740744 hasConceptScore W3121740744C4839761 @default.

• next