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The Arches Mass Function

Published online by Cambridge University Press:  31 January 2003

A. Stolte*
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
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Abstract

VLTI observations of individual, massive objects in dense star forming regions limited by crowding in conventional astronomy, can have impacts on the determination of the stellar mass spectrum, and test classical methods to derive the mass function.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2003

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