Hostname: page-component-5cf477f64f-r2nwp Total loading time: 0 Render date: 2025-04-03T03:02:58.874Z Has data issue: false hasContentIssue false
  • English
  • Français

Luminosity Classification of Be Stars by Balmer Line Narrow Band Photometry

Published online by Cambridge University Press:  14 August 2015

Wolfgang Zeuge
Wolfgang Zeuge*
Affiliation:
Hamburg Observatory, Gojenbergsweg 112, D-2050 Hamburg 80, FRG

Extract

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 absolute luminosity of most Be stars can be determined by using Balmer line narrow band photometry with an accuracy of about 0.4 mag. The few cases in which this method fails can be detected.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 37 - 40
Copyright
Copyright © Reidel 1982 

References

Literature

Abt, H.A., Golson, J.C.: 1966, Astrophys. J. 143, p. 306 Google Scholar
Crowford, D.L., Mander, J.: 1966, Astron. J. 71, p. 114 Google Scholar
Feinstein, A.: 1976, in IAU Symposium 70, Be and shell stars, ed. Slettebak, A. (D. Reidel, Dordrecht, Holland), p. 249 Google Scholar
Feinstein, A.: 1979, Astron. J. 84, p. 1713 CrossRefGoogle Scholar
Zeuge, W.: 1981, Google Scholar