Titlebook: Circumstellar Matter 1994; Proceedings of an In G. D. Watt,P. M. Williams Conference proceedings 1995 Springer Science+Business Media Dordr

黄瓜

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

爵士乐

temperate

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

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

作呕

门窗的侧柱

Contracture

http://image.papertrans.cn/c/image/226656.jpg

FISC