Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-26T18:23:17.065Z Has data issue: false hasContentIssue false
  • English
  • Français

Time Dependence of Balmer Progression in the Spectrum of HD 92207

Published online by Cambridge University Press:  12 April 2016

H.G. Groth
H.G. Groth*
Affiliation:
Inst. für Astronomie und Astrophysik, Universität München, München 80, West 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.

The radial velocities measured in the spectrum of HD 92207 (AO Ia+) show a Balmer progression, which varies considerably within one week and reverses within one month (or less). These observations give strong evidence, that at least in some parts of the atmosphere the velocity field reverses with time. (To be published in Astronomy and Astrophysics).

Type
2. Observed Properties of Stellar Turbulence
Information
International Astronomical Union Colloquium , Volume 51: Stellar Turbulence , 1980 , pp. 163
Copyright
Copyright © Springer-Verlag 1980