FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2097133096> ?p ?o ?g. }

• W2097133096 endingPage "665" @default.
• W2097133096 startingPage "657" @default.
• W2097133096 abstract "We investigate the properties of circumplanetary discs formed in three-dimensional, self-gravitating radiation hydrodynamical models of gas accretion by protoplanets. We determine disc sizes, scaleheights, and density and temperature profiles for different protoplanet masses, in solar nebulae of differing grain opacities. We find that the analytical prediction of circumplanetary disc radii in an evacuated gap (R_Hill/3) from Quillen & Trilling (1998) yields a good estimate for discs formed by high mass protoplanets. The radial density profiles of the circumplanetary discs may be described by power-laws between r^-2 and r^-3/2. We find no evidence for the ring-like density enhancements that have been found in some previous models of circumplanetary discs. Temperature profiles follow a ~r^-7/10 power-law regardless of protoplanet mass or nebula grain opacity. The discs invariably have large scaleheights (H/r > 0.2), making them thick in comparison with their encompassing circumstellar discs, and they show no flaring." @default.
• W2097133096 created "2016-06-24" @default.
• W2097133096 creator A5055139605 @default.
• W2097133096 creator A5061761792 @default.
• W2097133096 date "2009-08-01" @default.
• W2097133096 modified "2023-10-16" @default.
• W2097133096 title "Circumplanetary disc properties obtained from radiation hydrodynamical simulations of gas accretion by protoplanets" @default.
• W2097133096 cites W1616194406 @default.
• W2097133096 cites W1639285581 @default.
• W2097133096 cites W1654550887 @default.
• W2097133096 cites W1974486269 @default.
• W2097133096 cites W1978204777 @default.
• W2097133096 cites W1995864175 @default.
• W2097133096 cites W2024605337 @default.
• W2097133096 cites W2041389756 @default.
• W2097133096 cites W2042035263 @default.
• W2097133096 cites W2042607720 @default.
• W2097133096 cites W2046128110 @default.
• W2097133096 cites W2053721702 @default.
• W2097133096 cites W2066375046 @default.
• W2097133096 cites W2073799363 @default.
• W2097133096 cites W2074369638 @default.
• W2097133096 cites W2076730205 @default.
• W2097133096 cites W2076822660 @default.
• W2097133096 cites W2087070454 @default.
• W2097133096 cites W2102787996 @default.
• W2097133096 cites W2122237670 @default.
• W2097133096 cites W2128808878 @default.
• W2097133096 cites W2132781885 @default.
• W2097133096 cites W2142254839 @default.
• W2097133096 cites W2158458309 @default.
• W2097133096 cites W2161386047 @default.
• W2097133096 cites W2162003020 @default.
• W2097133096 cites W2168570318 @default.
• W2097133096 cites W3021622851 @default.
• W2097133096 cites W3098041279 @default.
• W2097133096 cites W3098885964 @default.
• W2097133096 cites W3100730144 @default.
• W2097133096 cites W3104870813 @default.
• W2097133096 cites W4302337765 @default.
• W2097133096 doi "https://doi.org/10.1111/j.1365-2966.2009.15002.x" @default.
• W2097133096 hasPublicationYear "2009" @default.
• W2097133096 type Work @default.
• W2097133096 sameAs 2097133096 @default.
• W2097133096 citedByCount "128" @default.
• W2097133096 countsByYear W20971330962012 @default.
• W2097133096 countsByYear W20971330962013 @default.
• W2097133096 countsByYear W20971330962014 @default.
• W2097133096 countsByYear W20971330962015 @default.
• W2097133096 countsByYear W20971330962016 @default.
• W2097133096 countsByYear W20971330962017 @default.
• W2097133096 countsByYear W20971330962018 @default.
• W2097133096 countsByYear W20971330962019 @default.
• W2097133096 countsByYear W20971330962020 @default.
• W2097133096 countsByYear W20971330962021 @default.
• W2097133096 countsByYear W20971330962022 @default.
• W2097133096 countsByYear W20971330962023 @default.
• W2097133096 crossrefType "journal-article" @default.
• W2097133096 hasAuthorship W2097133096A5055139605 @default.
• W2097133096 hasAuthorship W2097133096A5061761792 @default.
• W2097133096 hasBestOaLocation W20971330961 @default.
• W2097133096 hasConcept C120665830 @default.
• W2097133096 hasConcept C121332964 @default.
• W2097133096 hasConcept C1276947 @default.
• W2097133096 hasConcept C12853656 @default.
• W2097133096 hasConcept C2776401274 @default.
• W2097133096 hasConcept C2780909310 @default.
• W2097133096 hasConcept C44870925 @default.
• W2097133096 hasConcept C51244244 @default.
• W2097133096 hasConcept C60056205 @default.
• W2097133096 hasConcept C93436676 @default.
• W2097133096 hasConceptScore W2097133096C120665830 @default.
• W2097133096 hasConceptScore W2097133096C121332964 @default.
• W2097133096 hasConceptScore W2097133096C1276947 @default.
• W2097133096 hasConceptScore W2097133096C12853656 @default.
• W2097133096 hasConceptScore W2097133096C2776401274 @default.
• W2097133096 hasConceptScore W2097133096C2780909310 @default.
• W2097133096 hasConceptScore W2097133096C44870925 @default.
• W2097133096 hasConceptScore W2097133096C51244244 @default.
• W2097133096 hasConceptScore W2097133096C60056205 @default.
• W2097133096 hasConceptScore W2097133096C93436676 @default.
• W2097133096 hasIssue "2" @default.
• W2097133096 hasLocation W20971330961 @default.
• W2097133096 hasLocation W20971330962 @default.
• W2097133096 hasLocation W20971330963 @default.
• W2097133096 hasOpenAccess W2097133096 @default.
• W2097133096 hasPrimaryLocation W20971330961 @default.
• W2097133096 hasRelatedWork W1886511780 @default.
• W2097133096 hasRelatedWork W1984668662 @default.
• W2097133096 hasRelatedWork W1996937040 @default.
• W2097133096 hasRelatedWork W2024360329 @default.
• W2097133096 hasRelatedWork W2050942819 @default.
• W2097133096 hasRelatedWork W2097133096 @default.
• W2097133096 hasRelatedWork W249320820 @default.
• W2097133096 hasRelatedWork W2944587354 @default.
• W2097133096 hasRelatedWork W3104025681 @default.
• W2097133096 hasRelatedWork W4220769593 @default.
• W2097133096 hasVolume "397" @default.

• next