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The high-mass stellar IMF in different environments

Published online by Cambridge University Press:  01 August 2006

Pavel Kroupa
Pavel Kroupa*
Affiliation:
Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany email: [email protected]
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Abstract

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The massive-star IMF is found to be invariable. However, integrated IMFs probably depend on galactic mass.

Keywords

stars: luminosity functionmass functionstars: pre–main-sequence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 208
Copyright
Copyright © International Astronomical Union 2007

References

Adams, F. C., & Fatuzzo, M. 1996, ApJ, 464, 256CrossRefGoogle Scholar
Bonnell, I. A., Larson, R. B., & Zinnecker, H. 2006, in: Reipurth, B., Jewitt, D. & Keil, K. (eds.), Protostars and Planets V (Tucson: Univ. Arizona Press), p. 951Google Scholar
Weidner, C., & Kroupa, P. 2006, MNRAS, 365, 1333CrossRefGoogle Scholar
Larson, R. B. 1998, MNRAS, 301, 569CrossRefGoogle Scholar
Massey, P. 2003, ARAA, 41, 15CrossRefGoogle Scholar
Salpeter, E. E. 1955, ApJ, 121, 161CrossRefGoogle Scholar