黄瓜
发表于 2025-3-25 07:06:31
Klaudius Heda,Klaus Heine,Erich Oltmanns time-dependent radio sources which may be evidence for proto-stars losing their magnetic fields, and a `bullet’ which appears to be the head of a high velocity jet which causes the entrainment of molecular outflows.
Eviction
发表于 2025-3-25 11:16:20
http://reply.papertrans.cn/23/2267/226656/226656_22.png
爵士乐
发表于 2025-3-25 13:37:11
http://reply.papertrans.cn/23/2267/226656/226656_23.png
temperate
发表于 2025-3-25 18:47:52
Observations of Disks around Protostellar Sources with Nobeyama Millimeter Array shows that the 98 GHz continuum emission tends to be weaker for embedded sources than for visible T Tauri stars, which is consistent with our previous interpretation of disk formation. Direct observations of the formation of a centrifugally supported viscous accretion disk around HL Tau is discussed.
aplomb
发表于 2025-3-25 22:28:22
Infrared CO Emission and Disks around Young Starstellar disks around young stars. The CO emission flux and the detailed shape of the overtone bands are well matched by simple Keplerian disk models. A brief overview of the use of infrared CO emission as a diagnostic of the kinematics and conditions of gas in the inner disks of young stars is presented.
聪明
发表于 2025-3-26 03:27:57
http://reply.papertrans.cn/23/2267/226656/226656_26.png
作呕
发表于 2025-3-26 04:20:33
http://reply.papertrans.cn/23/2267/226656/226656_27.png
门窗的侧柱
发表于 2025-3-26 10:56:20
http://reply.papertrans.cn/23/2267/226656/226656_28.png
Contracture
发表于 2025-3-26 16:16:52
http://image.papertrans.cn/c/image/226656.jpg
FISC
发表于 2025-3-26 18:43:51
http://reply.papertrans.cn/23/2267/226656/226656_30.png