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High-precision continuum rectification * : Towards an Abundance Analysis of Be and Bn Stars

  • M. Kolb (a1) and D. Baade (a1)

Abstract

We sketch a new method for the accurate flux calibration and normalization of stellar spectra. This is of particular importance for the analysis of rapidly rotating early–type stars. Some preliminary log g determinations by profile fitting of H γ are presented.

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* Based on observations at the European Southern Observatory, La Silla, Chile

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