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Dust evolution in photoevaporating protoplanetary disks

Proceedings of the International Astronomical Union (2006) 2(S237) 455
DOI: 10.1017/S1743921307002438
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Abstract

We construct a model of the physical structure of photoevaporating protoplanetary disks, and numerically calculate the coagulation and settling/evaporating process of dust particles in the disks. Our result show that (sub)micron-sized-dust-particles could evaporate with the gas, which leads to dispersal of infrared excess radiation from the disks. © 2007 International Astronomical Union.

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APA

Nomura, H., Aikawa, Y., Inutsuka, S., & Nakagawa, Y. (2006). Dust evolution in photoevaporating protoplanetary disks. In Proceedings of the International Astronomical Union (Vol. 2, p. 455). Cambridge University Press. https://doi.org/10.1017/S1743921307002438

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