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Star formation in CHA T1

Published online by Cambridge University Press:  04 August 2017

P. R. Wesselius ,
R. Assendorp  and
H. Roede
P. R. Wesselius
Affiliation:
Space Research, P.O. Box 800, 9700 AY Groningen, The Netherlands
R. Assendorp
Affiliation:
Space Research, P.O. Box 800, 9700 AY Groningen, The Netherlands
H. Roede
Affiliation:
Space Research, P.O. Box 800, 9700 AY Groningen, The Netherlands

Abstract

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In a region of 0.4 × 0.5 pc around HD 97300 the amount of mass in gas and dust is < 16 M⊙, while the stellar mass is 6–9 M⊙. Thus in this core of a collapsing cloud (Cha T1) several stars have been formed in a very efficient way.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 95 - 96
Copyright
Copyright © Reidel 1987 

References

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