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dc.contributor.author Lyra, Wladimir
dc.date.accessioned 2017-10-11T21:49:19Z
dc.date.available 2017-10-11T21:49:19Z
dc.date.issued 2012
dc.identifier.citation Lyra, W. (2012). Formation and Retention of Planets in Protoplanetary Disks (Vol. 1667, p. 6310). Presented at the Asteroids, Comets, Meteors 2012. Retrieved from http://adsabs.harvard.edu/abs/2012LPICo1667.6310L en_US
dc.identifier.uri http://hdl.handle.net/10211.3/197068
dc.description.abstract This work presents 3D resistive magnetohydrodynamical models of the solar nebula, showing that the region between magnetically active and dead zones is prone to the excitation of vortices, that effectively form planetary embryos of Moon to Mars mass. en_US
dc.language.iso en en_US
dc.publisher Asteroids, Comets, Meteors 2012 en_US
dc.relation.uri http://adsabs.harvard.edu/abs/2012LPICo1667.6310L en_US
dc.subject magnetohydrodynamical models en_US
dc.subject solar nebula en_US
dc.subject magnetic fields en_US
dc.subject astronomy en_US
dc.subject astrophysics en_US
dc.title Formation and Retention of Planets in Protoplanetary Disks en_US
dc.type conference paper en_US


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