Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk?

Details Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk? Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk?

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005icar..176..220s&link_type=abstract

Icarus, Volume 176, Issue 1, p. 220-223.

Astronomy and Astrophysics

Astrophysics

13

Scientific paper

Sekiya and Takeda [2003, Earth Planets Space 55, 263 269] showed that the hydrodynamic gas flow around a dust aggregate larger than the mean free path of gas molecules prevents the growth of the body. In contrast to Wurm et al. [2004, Astrophys. J. 606, 983 987], we argue that this conclusion is not altered even if we take account of the effect of the flow through a porous dust aggregate.

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