Physics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..130a4012h&link_type=abstract
Physica Scripta, Volume 130, Issue , pp. 014012 (2008).
Physics
3
Scientific paper
I discuss some recent estimates of protoplanetary disk masses from dust emission, and suggest that masses have been systematically underestimated. I also consider the implications of recent results on the outbursting FU Ori objects, which demonstrate the need for substantial amounts of mass in disks within 1 AU, at least at early evolutionary stages. These considerations lend more weight to suggestions that protoplanetary disks have relatively massive 'dead zones', which may aid in the formation of the so-called 'transitional disk' systems, objects in which the inner disk has been strongly cleared of small dust even though the outer disk is very substantial.
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