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Theory of protoplanetary disks
Astrophysics and Space Science, 1995The evolution of protoplanetary disks around young stars is briefly reviewed. The most important physical mechanisms that drive the mass accretion are gravitational, magnetic, and thermal convective instabilities. These mechanisms are dominant in different regions of the disk and at different evolutionary epochs.
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Chemistry of Protoplanetary Disks
2004We consider the chemistry occurring in protoplanetary disks and its possible contribution to the organic inventory of primitive solar system bodies. First, we outline the main physical and chemical processes associated with the formation of solar-type stars and their accretion disks.
A.J. Markwickan, Steven B. Charnley
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Chondrules and the Protoplanetary Disk
Physics of the Earth and Planetary Interiors, 1997openaire +2 more sources