Titlebook: Dust-Gas Instabilities in Protoplanetary Disks; Toward Understanding Ryosuke Tominaga Book 2022 The Editor(s) (if applicable) and The Autho

homeostasis

Positive Youth Development in Chinaing secular gravitational instability. The previous dust-gas instabilities require super-solar metallicity and large dust grains whose dimensionless stopping time is 0.1–1. However, dust coagulation models have shown that dust growth proceeds in inside-out manner and the resulting radial drift cause

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When Will a Repost Cascade Settle Down?here planetesimals form are not smooth profile as assumed in the classical standard theory but quite structured. Especially, dust rings and gaps have been frequently observed, which might be the key to explain dust growth toward planetesimals in protoplanetary disks. In this thesis, we investigate d

性學(xué)院

Observe

Carmen Buzea,Radosveta Dimitrova under debate. In this chapter, we briefly review disk formation from a molecular cloud core, basic dust dynamics in a disk, and recent high-resolution disk observations with Atacama Large Millimeter/submillimeter Array (ALMA) that provides hints to reveal planetesimal formation.

上坡

雪白

Introduction, under debate. In this chapter, we briefly review disk formation from a molecular cloud core, basic dust dynamics in a disk, and recent high-resolution disk observations with Atacama Large Millimeter/submillimeter Array (ALMA) that provides hints to reveal planetesimal formation.

膝蓋

,Summary and?Future Prospects,ust-gas instabilities that have potential to explain dust ring formation and planetesimal formation based on linear analyses and numerical simulations. In this chapter, we summarize the studies presented in this thesis and describe future prospects.

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肌肉

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