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High-precision continuum rectification*: Towards an Abundance Analysis of Be and Bn Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
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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.
- Type
- 6. Be Stars: Circumstellar Environment
- Information
- Copyright
- Copyright © Kluwer 1994