FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100406661> ?p ?o ?g. }

• W3100406661 endingPage "16" @default.
• W3100406661 startingPage "16" @default.
• W3100406661 abstract "Recent years have seen growing interest in the streaming instability as a candidate mechanism to produce planetesimals. However, these investigations have been limited to small-scale simulations. We now present the results of a global protoplanetary disk evolution model that incorporates planetesimal formation by the streaming instability, along with viscous accretion, photoevaporation by EUV, FUV, and X-ray photons, dust evolution, the water ice line, and stratified turbulence. Our simulations produce massive (60-130 $M_oplus$) planetesimal belts beyond 100 au and up to $sim 20 M_oplus$ of planetesimals in the middle regions (3-100 au). Our most comprehensive model forms 8 $M_oplus$ of planetesimals inside 3 au, where they can give rise to terrestrial planets. The planetesimal mass formed in the inner disk depends critically on the timing of the formation of an inner cavity in the disk by high-energy photons. Our results show that the combination of photoevaporation and the streaming instability are efficient at converting the solid component of protoplanetary disks into planetesimals. Our model, however, does not form enough early planetesimals in the inner and middle regions of the disk to give rise to giant planets and super-Earths with gaseous envelopes. Additional processes such as particle pileups and mass loss driven by MHD winds may be needed to drive the formation of early planetesimal generations in the planet forming regions of protoplanetary disks." @default.
• W3100406661 created "2020-11-23" @default.
• W3100406661 creator A5012735923 @default.
• W3100406661 creator A5031569510 @default.
• W3100406661 creator A5068874155 @default.
• W3100406661 creator A5083518430 @default.
• W3100406661 date "2017-04-10" @default.
• W3100406661 modified "2023-10-16" @default.
• W3100406661 title "Planetesimal Formation by the Streaming Instability in a Photoevaporating Disk" @default.
• W3100406661 cites W1542275802 @default.
• W3100406661 cites W1848194890 @default.
• W3100406661 cites W1942002525 @default.
• W3100406661 cites W1972082652 @default.
• W3100406661 cites W1985707679 @default.
• W3100406661 cites W1987843370 @default.
• W3100406661 cites W1988498914 @default.
• W3100406661 cites W1990646059 @default.
• W3100406661 cites W1994277384 @default.
• W3100406661 cites W1994358959 @default.
• W3100406661 cites W2000421598 @default.
• W3100406661 cites W2000657683 @default.
• W3100406661 cites W2005271140 @default.
• W3100406661 cites W2011177045 @default.
• W3100406661 cites W2017734128 @default.
• W3100406661 cites W2018776416 @default.
• W3100406661 cites W2020204680 @default.
• W3100406661 cites W2031065107 @default.
• W3100406661 cites W2031513034 @default.
• W3100406661 cites W2034147949 @default.
• W3100406661 cites W2034608771 @default.
• W3100406661 cites W2041172302 @default.
• W3100406661 cites W2048461140 @default.
• W3100406661 cites W2054844325 @default.
• W3100406661 cites W2057006726 @default.
• W3100406661 cites W2063887564 @default.
• W3100406661 cites W2068433364 @default.
• W3100406661 cites W2075076813 @default.
• W3100406661 cites W2080426384 @default.
• W3100406661 cites W2080480291 @default.
• W3100406661 cites W2085012582 @default.
• W3100406661 cites W2093494526 @default.
• W3100406661 cites W2099171476 @default.
• W3100406661 cites W2102049225 @default.
• W3100406661 cites W2106595367 @default.
• W3100406661 cites W2107333743 @default.
• W3100406661 cites W2108530185 @default.
• W3100406661 cites W2112716743 @default.
• W3100406661 cites W2114282862 @default.
• W3100406661 cites W2116952160 @default.
• W3100406661 cites W2118339586 @default.
• W3100406661 cites W2128689994 @default.
• W3100406661 cites W2132117032 @default.
• W3100406661 cites W2140083426 @default.
• W3100406661 cites W2153970052 @default.
• W3100406661 cites W2156621121 @default.
• W3100406661 cites W2158129300 @default.
• W3100406661 cites W2164235908 @default.
• W3100406661 cites W2194639733 @default.
• W3100406661 cites W2290726778 @default.
• W3100406661 cites W2594921500 @default.
• W3100406661 cites W2947592794 @default.
• W3100406661 cites W3098454390 @default.
• W3100406661 cites W3099125925 @default.
• W3100406661 cites W3099213932 @default.
• W3100406661 cites W3099474760 @default.
• W3100406661 cites W3099936221 @default.
• W3100406661 cites W3100354223 @default.
• W3100406661 cites W3100521337 @default.
• W3100406661 cites W3100530613 @default.
• W3100406661 cites W3100712340 @default.
• W3100406661 cites W3100998258 @default.
• W3100406661 cites W3101442198 @default.
• W3100406661 cites W3102115841 @default.
• W3100406661 cites W3102418355 @default.
• W3100406661 cites W3102581452 @default.
• W3100406661 cites W3103069457 @default.
• W3100406661 cites W3103603022 @default.
• W3100406661 cites W3104702592 @default.
• W3100406661 cites W3105272212 @default.
• W3100406661 cites W3105591496 @default.
• W3100406661 cites W3105647453 @default.
• W3100406661 cites W3105714136 @default.
• W3100406661 cites W3106083296 @default.
• W3100406661 cites W3124152154 @default.
• W3100406661 cites W3124369829 @default.
• W3100406661 cites W3147751559 @default.
• W3100406661 cites W4292332867 @default.
• W3100406661 doi "https://doi.org/10.3847/1538-4357/aa6932" @default.
• W3100406661 hasPublicationYear "2017" @default.
• W3100406661 type Work @default.
• W3100406661 sameAs 3100406661 @default.
• W3100406661 citedByCount "133" @default.
• W3100406661 countsByYear W31004066612017 @default.
• W3100406661 countsByYear W31004066612018 @default.
• W3100406661 countsByYear W31004066612019 @default.
• W3100406661 countsByYear W31004066612020 @default.
• W3100406661 countsByYear W31004066612021 @default.
• W3100406661 countsByYear W31004066612022 @default.

• next