Morphology of Protostellar Cores from RUN1 at t=0.4213

~5 pc overdense structures of supersonic turbulence in a molecular cloud
CubeA.jpg	CubeB.jpg	CubeC1.jpg	CubeC2.jpg	CubeC3.jpg
~0.02 pc a chain of five cores fragmented out of a single dense filament
Chain.jpg
~0.01 pc cores No. 2, 3, and 4 from different view points
Core234A.jpg	Core234B.jpg	Core234C.jpg	Core234D.jpg	Core234E.jpg	Core234F.jpg
~500 a.u. volumertic rendering and density PDF for core No. 1
Core1edgeA.jpg	Core1edgeB.jpg	Core1edgeC.jpg	Core1faceA.jpg	Core1faceB.jpg
Core1faceC.jpg	Core1faceD.jpg	Core1faceE.jpg	Core1faceF.jpg	Core1PDF.jpg
core No. 2
Core2edge.jpg	Core2face.jpg
a small core No. 5
Core5edge.jpg	Core5face.jpg
an irregular core No. 6
Core6edge.jpg	Core6face.jpg
a tight triple system of interacting collapsed cores: "core No. 7"
Core7A.jpg	Core7B.jpg	Core7C.jpg	Core7D.jpg	Core7E.jpg
Core7F.jpg	Core7G.jpg	Core7H.jpg	Core7I.jpg	Core7J.jpg
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Last modified: Sep 20, 2004 Comments to: akritsuk@ucsd.edu