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Astron. Astrophys. 361, 1191 (2000)

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Hard X-rays emitted by starbursts as predicted by population synthesis models including a realistic fraction of interacting binaries

J. Van Bever and D. Vanbeveren

Vrije Universiteit Brussel, Astrophysical Institute, Pleinlaan 2, 1050 Brussels, Belgium (jvbever@vub.ac.be; dvbevere@vub.ac.be)

Astron. Astrophys. 358, 462-470 (2000)

Due to an unfortunate error the wrong Fig. 11 has been inserted. Following this page the complete paper will be printed once again including the correct Fig. 11.

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© European Southern Observatory (ESO) 2000

Online publication: October 10, 2000