Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100225862> ?p ?o ?g. }
- W3100225862 endingPage "L2" @default.
- W3100225862 startingPage "L2" @default.
- W3100225862 abstract "We report on the discovery of correlations between dust and CO gas tracers of the 0.1-10 au region in planet-forming disks around young intermediate-mass stars. The abundance of refractory elements on stellar photospheres decreases as the location of hot CO gas emission recedes to larger disk radii, and as the near-infrared excess emission from hot dust in the inner disk decreases. The linked behavior between these observables demonstrates that the recession of infrared CO emission to larger disk radii traces an inner disk region where dust is being depleted. We also find that Herbig disk cavities have either low (~ 5-10 %) or high (~ 20-35 %) near-infrared excess, a dichotomy that has not been captured by the classic definition of pre-transitional disks." @default.
- W3100225862 created "2020-11-23" @default.
- W3100225862 creator A5030468546 @default.
- W3100225862 creator A5039341024 @default.
- W3100225862 creator A5063164095 @default.
- W3100225862 creator A5065010090 @default.
- W3100225862 creator A5076646665 @default.
- W3100225862 creator A5081520912 @default.
- W3100225862 creator A5086191109 @default.
- W3100225862 date "2018-01-01" @default.
- W3100225862 modified "2023-09-30" @default.
- W3100225862 title "Observing the linked depletion of dust and CO gas at 0.1–10 au in disks of intermediate-mass stars" @default.
- W3100225862 cites W2006224949 @default.
- W3100225862 cites W2018164398 @default.
- W3100225862 cites W2025788510 @default.
- W3100225862 cites W2047775701 @default.
- W3100225862 cites W2056067779 @default.
- W3100225862 cites W2060648965 @default.
- W3100225862 cites W2068008066 @default.
- W3100225862 cites W2068474102 @default.
- W3100225862 cites W2095705361 @default.
- W3100225862 cites W2107656875 @default.
- W3100225862 cites W2118309316 @default.
- W3100225862 cites W2118522798 @default.
- W3100225862 cites W2125314121 @default.
- W3100225862 cites W2131011360 @default.
- W3100225862 cites W2159258911 @default.
- W3100225862 cites W2171291743 @default.
- W3100225862 cites W2174187778 @default.
- W3100225862 cites W2211049752 @default.
- W3100225862 cites W2217709223 @default.
- W3100225862 cites W2301347023 @default.
- W3100225862 cites W2513697673 @default.
- W3100225862 cites W2519589111 @default.
- W3100225862 cites W2585137288 @default.
- W3100225862 cites W2604724397 @default.
- W3100225862 cites W2605057281 @default.
- W3100225862 cites W2607362108 @default.
- W3100225862 cites W2619573834 @default.
- W3100225862 cites W2763043108 @default.
- W3100225862 cites W2763541541 @default.
- W3100225862 cites W3099093368 @default.
- W3100225862 cites W3099296325 @default.
- W3100225862 cites W3099879872 @default.
- W3100225862 cites W3099976733 @default.
- W3100225862 cites W3100228619 @default.
- W3100225862 cites W3100314980 @default.
- W3100225862 cites W3100515644 @default.
- W3100225862 cites W3101040884 @default.
- W3100225862 cites W3102186960 @default.
- W3100225862 cites W3102726572 @default.
- W3100225862 cites W3102997874 @default.
- W3100225862 cites W3103681827 @default.
- W3100225862 cites W3103896847 @default.
- W3100225862 cites W3103938748 @default.
- W3100225862 cites W3104280308 @default.
- W3100225862 cites W3105384870 @default.
- W3100225862 cites W3105578058 @default.
- W3100225862 cites W3105673385 @default.
- W3100225862 cites W3106503074 @default.
- W3100225862 cites W3123911708 @default.
- W3100225862 cites W3125109692 @default.
- W3100225862 cites W4289259160 @default.
- W3100225862 cites W4292406868 @default.
- W3100225862 cites W4297902100 @default.
- W3100225862 cites W4298846666 @default.
- W3100225862 cites W4300579480 @default.
- W3100225862 doi "https://doi.org/10.1051/0004-6361/201732034" @default.
- W3100225862 hasPublicationYear "2018" @default.
- W3100225862 type Work @default.
- W3100225862 sameAs 3100225862 @default.
- W3100225862 citedByCount "29" @default.
- W3100225862 countsByYear W31002258622018 @default.
- W3100225862 countsByYear W31002258622019 @default.
- W3100225862 countsByYear W31002258622020 @default.
- W3100225862 countsByYear W31002258622021 @default.
- W3100225862 countsByYear W31002258622022 @default.
- W3100225862 countsByYear W31002258622023 @default.
- W3100225862 crossrefType "journal-article" @default.
- W3100225862 hasAuthorship W3100225862A5030468546 @default.
- W3100225862 hasAuthorship W3100225862A5039341024 @default.
- W3100225862 hasAuthorship W3100225862A5063164095 @default.
- W3100225862 hasAuthorship W3100225862A5065010090 @default.
- W3100225862 hasAuthorship W3100225862A5076646665 @default.
- W3100225862 hasAuthorship W3100225862A5081520912 @default.
- W3100225862 hasAuthorship W3100225862A5086191109 @default.
- W3100225862 hasBestOaLocation W31002258621 @default.
- W3100225862 hasConcept C121332964 @default.
- W3100225862 hasConcept C1276947 @default.
- W3100225862 hasConcept C150846664 @default.
- W3100225862 hasConcept C158355884 @default.
- W3100225862 hasConcept C2779760567 @default.
- W3100225862 hasConcept C44870925 @default.
- W3100225862 hasConcept C51244244 @default.
- W3100225862 hasConcept C8865038 @default.
- W3100225862 hasConceptScore W3100225862C121332964 @default.
- W3100225862 hasConceptScore W3100225862C1276947 @default.
- W3100225862 hasConceptScore W3100225862C150846664 @default.