Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-25T17:59:57.896Z Has data issue: false hasContentIssue false

Summary and concluding remarks

Published online by Cambridge University Press:  01 May 2007

Immo Appenzeller*
Affiliation:
University of Heidelberg, Landessternwarte, Königstuhl, D 69117 Heidelberg, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Heitsch, F., Hartmann, L., Slyz, A. D., Devrient, J. E., Burkert, A. 2006, BAAS 209, 1715Google Scholar
Herbig, G. H. 1977, in: de Jong, T. & Maeder, A. (eds.), in: Proc. IAU Symposium 75 on Star Formation, (Dordrecht: D. Reidel) p. 283Google Scholar
Jappsen, A.-K., Klessen, R. S., Larson, R. B., Li, Y., Mac Low, M.-M. 2005, A&A 435, 611Google Scholar
Walker, M.F. 1972, ApJ 175, 89CrossRefGoogle Scholar