Titlebook: Disks and Outflows Around Young Stars; Proceedings of a Con Steven Beckwith,Jakob Staude,Antonella Natta Conference proceedings 1996 Spring

骇人

Numerical simulations of the formation of binary and multiple protostellar disks, starting from dyn

圆木可阻碍

Multiplicity in the Opiuchus and Taurus star forming regions,

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航海太平洋

佛刊

Definitive

BRAVE

Factorable

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MEEK

High resolution observations of disks around protostellar sources with the Nobeyama Millimeter Arrant with our previous interpretation of protoplanetary disk formation. The CS gas around L1489 and IRAS 04365+2535 show disk-like structures of ∼1000 AU in radius. A .CO observation of HL Tau indicates direct evidence of dynamical infalling motion. We discuss the formation of a centrifugally supported viscous accretion disk around HL Tau.