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Dust emission from star forming clouds: a progress report

Published online by Cambridge University Press:  03 August 2017

P. G. Mezger ,
A. Sievers  and
R. Zylka
P. G. Mezger
Affiliation:
MPIfR bolometer group ∗ Max—Planck—Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn 1
A. Sievers
Affiliation:
MPIfR bolometer group ∗ Max—Planck—Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn 1
R. Zylka
Affiliation:
MPIfR bolometer group ∗ Max—Planck—Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn 1

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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.

Type
Small Scale Structure
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 245 - 257
Copyright
Copyright © Kluwer 1991 

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