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- W4239478809 abstract "Model computations of protostellar evolution depend very strongly on the initial conditions: Fragmentation of massive cloud cores or coagulation of substellar condensations, the physical state of gas and dust (e.g. the formation of ice-mantles and grain coagulation), the presence of magnetic fields and its effect on gas and dust, and the formation of accretion disks as a consequence of an initial angular momentum of the protostellar condensation. The MPIfR bolometer group together with the molecular spectroscopists R. Mauersberger and T.L. Wilson have embarked on a program aimed at the exploration of the earliest evolutionary stages of high- and low-mass star formation. Here follows a brief progress report." @default.
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- W4239478809 date "1991-01-01" @default.
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- W4239478809 title "Dust emission from star forming clouds: a progress report" @default.
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- W4239478809 doi "https://doi.org/10.1017/s0074180900198973" @default.
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