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Summary and concluding remarks

Published online by Cambridge University Press:  01 May 2007

Immo Appenzeller
Immo Appenzeller*
Affiliation:
University of Heidelberg, Landessternwarte, Königstuhl, D 69117 Heidelberg, Germany email: I.Appenzeller@lsw.uni-heidelberg.de
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Abstract

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This symposium was characterized by an intense exchange of new information and by lively discussions on many aspects of the formation and early evolution of low-mass stars. The observational data presented at this meeting, obtained in spectral regions ranging from X-rays to submm waves, were found to be remarkably consistent with the current magnetospheric disc-accretion paradigm for young stellar objects. But there remain open questions, and a full understanding of the star-formation process will require much additional work.

Keywords

Stars: formationstars: pre–main-sequenceISM: jets and outflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S243: Star-Disk Interaction in Young Stars , May 2007 , pp. 365 - 369
Copyright
Copyright © International Astronomical Union 2007

References

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