Hostname: page-component-77c89778f8-9q27g Total loading time: 0 Render date: 2024-07-16T19:42:14.799Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  26 May 2016

M. Kolb
Affiliation:
European Southern Observatory Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany
D. Baade
Affiliation:
European Southern Observatory Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Kluwer 1994