Formation and Retention of Planets in Protoplanetary Disks

dc.contributor.author	Lyra, Wladimir	en
dc.date.accessioned	2017-10-11T21:49:19Z
dc.date.available	2017-10-11T21:49:19Z
dc.date.issued	2012	en
dc.identifier.citation	LPI Contribution 1667. (2012)	en
dc.identifier.other	http://adsabs.harvard.edu/abs/2012LPICo1667.6310L	en
dc.identifier.uri	http://hdl.handle.net/10211.3/197068	en
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
dc.language.iso	en	en
dc.publisher	Asteroids, Comets, Meteors 2012	en
dc.subject	magnetohydrodynamical models	en
dc.subject	solar nebula	en
dc.subject	magnetic fields	en
dc.subject	astronomy	en
dc.subject	astrophysics	en
dc.title	Formation and Retention of Planets in Protoplanetary Disks	en
dc.type	Conference paper or proceedings	en

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