FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104012775> ?p ?o ?g. }

• W3104012775 endingPage "50" @default.
• W3104012775 startingPage "50" @default.
• W3104012775 abstract "The amount of dust present in circumstellar disks is expected to steadily decrease with age due to the growth from μm-sized particles to planetesimals and planets. Mature circumstellar disks, however, can be observed to contain significant amounts of dust and possess high dust-to-gas ratios. Using HD 163296 as our case study, we explore how the formation of giant planets in disks can create the conditions for collisionally rejuvenating the dust population, halting or reversing the expected trend. We combine N-body simulations with statistical methods and impact scaling laws to estimate the dynamical and collisional excitation of the planetesimals due to the formation of HD 163296's giant planets. We show that this process creates a violent collisional environment across the disk that can inject collisionally produced second-generation dust into it, significantly contributing to the observed dust-to-gas ratio. The spatial distribution of the dust production can explain the observed local enrichments in HD 163296's inner regions. The results obtained for HD 163296 can be extended to any disk with embedded forming giant planets and may indicate a common evolutionary stage in the life of such circumstellar disks. Furthermore, the dynamical excitation of the planetesimals could result in the release of transient, nonequilibrium gas species like H2O, CO2, NH3, and CO in the disk due to ice sublimation during impacts and, due to the excited planetesimals being supersonic with respect to the gas, could produce bow shocks in the latter that could heat it and cause a broadening of its emission lines." @default.
• W3104012775 created "2020-11-23" @default.
• W3104012775 creator A5028320043 @default.
• W3104012775 creator A5042629640 @default.
• W3104012775 creator A5058111055 @default.
• W3104012775 creator A5087288499 @default.
• W3104012775 date "2019-05-23" @default.
• W3104012775 modified "2023-10-18" @default.
• W3104012775 title "Dust-to-gas Ratio Resurgence in Circumstellar Disks Due to the Formation of Giant Planets: The Case of HD 163296" @default.
• W3104012775 cites W147232447 @default.
• W3104012775 cites W1613647566 @default.
• W3104012775 cites W1624814720 @default.
• W3104012775 cites W1667166397 @default.
• W3104012775 cites W1970508912 @default.
• W3104012775 cites W1974335835 @default.
• W3104012775 cites W1984592680 @default.
• W3104012775 cites W1984963133 @default.
• W3104012775 cites W1991574390 @default.
• W3104012775 cites W1998757246 @default.
• W3104012775 cites W2011037261 @default.
• W3104012775 cites W2019579421 @default.
• W3104012775 cites W2024147941 @default.
• W3104012775 cites W2041875623 @default.
• W3104012775 cites W2057740347 @default.
• W3104012775 cites W2067156389 @default.
• W3104012775 cites W2074041846 @default.
• W3104012775 cites W2080414318 @default.
• W3104012775 cites W2088702447 @default.
• W3104012775 cites W2090205023 @default.
• W3104012775 cites W2090949706 @default.
• W3104012775 cites W2114282862 @default.
• W3104012775 cites W2115618550 @default.
• W3104012775 cites W2118828158 @default.
• W3104012775 cites W2128308786 @default.
• W3104012775 cites W2134217601 @default.
• W3104012775 cites W2146348165 @default.
• W3104012775 cites W2322812581 @default.
• W3104012775 cites W2398572489 @default.
• W3104012775 cites W2561823294 @default.
• W3104012775 cites W2591665485 @default.
• W3104012775 cites W2604724397 @default.
• W3104012775 cites W2728619065 @default.
• W3104012775 cites W2767778740 @default.
• W3104012775 cites W2795896084 @default.
• W3104012775 cites W2798336535 @default.
• W3104012775 cites W2804872128 @default.
• W3104012775 cites W2809003569 @default.
• W3104012775 cites W2903886915 @default.
• W3104012775 cites W2913321873 @default.
• W3104012775 cites W2952860843 @default.
• W3104012775 cites W3098485869 @default.
• W3104012775 cites W3100200288 @default.
• W3104012775 cites W3100441347 @default.
• W3104012775 cites W3101187304 @default.
• W3104012775 cites W3101599961 @default.
• W3104012775 cites W3102054143 @default.
• W3104012775 cites W3102083771 @default.
• W3104012775 cites W3103603022 @default.
• W3104012775 cites W3105139946 @default.
• W3104012775 cites W3105591496 @default.
• W3104012775 cites W3105972254 @default.
• W3104012775 cites W3106110347 @default.
• W3104012775 cites W3124210067 @default.
• W3104012775 doi "https://doi.org/10.3847/1538-4357/ab18f5" @default.
• W3104012775 hasPublicationYear "2019" @default.
• W3104012775 type Work @default.
• W3104012775 sameAs 3104012775 @default.
• W3104012775 citedByCount "14" @default.
• W3104012775 countsByYear W31040127752020 @default.
• W3104012775 countsByYear W31040127752021 @default.
• W3104012775 countsByYear W31040127752022 @default.
• W3104012775 countsByYear W31040127752023 @default.
• W3104012775 crossrefType "journal-article" @default.
• W3104012775 hasAuthorship W3104012775A5028320043 @default.
• W3104012775 hasAuthorship W3104012775A5042629640 @default.
• W3104012775 hasAuthorship W3104012775A5058111055 @default.
• W3104012775 hasAuthorship W3104012775A5087288499 @default.
• W3104012775 hasBestOaLocation W31040127751 @default.
• W3104012775 hasConcept C100905312 @default.
• W3104012775 hasConcept C121332964 @default.
• W3104012775 hasConcept C1276947 @default.
• W3104012775 hasConcept C12853656 @default.
• W3104012775 hasConcept C163479331 @default.
• W3104012775 hasConcept C173740370 @default.
• W3104012775 hasConcept C190841160 @default.
• W3104012775 hasConcept C2780118271 @default.
• W3104012775 hasConcept C2780909310 @default.
• W3104012775 hasConcept C44870925 @default.
• W3104012775 hasConcept C51244244 @default.
• W3104012775 hasConcept C75876914 @default.
• W3104012775 hasConcept C87355193 @default.
• W3104012775 hasConcept C8865038 @default.
• W3104012775 hasConcept C94130837 @default.
• W3104012775 hasConceptScore W3104012775C100905312 @default.
• W3104012775 hasConceptScore W3104012775C121332964 @default.
• W3104012775 hasConceptScore W3104012775C1276947 @default.
• W3104012775 hasConceptScore W3104012775C12853656 @default.
• W3104012775 hasConceptScore W3104012775C163479331 @default.

• next