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Dead zones and the formation of jovian planets
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Dead zones and the formation of jovian planets

Abstract

Planets may complete their accretion when they become massive enough to open gaps in the face of disk viscosity. The prediction that gap-opening mass is related to disk viscosity implies that planetary masses are sensitive to the degree of ionization of the disk in the expected situation that viscosity is driven by magnetoturbulence by the well-known MRI instability. We show that in dead zones - poorly ionized regions wherein the MRI instability is unable to develop - only planets of terrestrial mass can form while Jovian planets form outside such regions. Dead zones extend out to 5-20 AU depending upon the disk column density.

Authors

Pudritz RE; Matsumura S

Volume

22

Pagination

pp. 108-112

Publication Date

December 1, 2004

Conference proceedings

Revista Mexicana De Astronomia Y Astrofisica Serie De Conferencias

ISSN

1405-2059

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