骇人
发表于 2025-3-28 17:09:32
Numerical simulations of the formation of binary and multiple protostellar disks, starting from dyn
圆木可阻碍
发表于 2025-3-28 22:06:00
Multiplicity in the Opiuchus and Taurus star forming regions,
关节炎
发表于 2025-3-29 00:12:09
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航海太平洋
发表于 2025-3-29 06:40:43
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佛刊
发表于 2025-3-29 10:13:07
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Definitive
发表于 2025-3-29 11:28:41
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BRAVE
发表于 2025-3-29 16:23:21
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Factorable
发表于 2025-3-29 20:47:27
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鞭打
发表于 2025-3-30 01:13:20
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MEEK
发表于 2025-3-30 04:48:10
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.