Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-11T12:17:41.803Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectral Energy Distribution of Be Stars

Published online by Cambridge University Press:  23 September 2016

Dieter Kaiser  and
Reinhard W. Hanuschik
Dieter Kaiser
Affiliation:
Astronomisches Institut, Ruhr-Universität Bochum, Postfach 10 21 48, D-4630 Bochum 1, FRG
Reinhard W. Hanuschik
Affiliation:
Astronomisches Institut, Ruhr-Universität Bochum, Postfach 10 21 48, D-4630 Bochum 1, 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.

During two observation periods in Nov./Dec. 1981 and April/ May 1985, absolute spectral energy distributions of 41 southern and equatorial Be stars were photometrically measured at 10 Å spectral resolution in the wavelength range between 3200 Å and 8500 Å, using the scanning spectrophotometer attached to the 61 cm telescope of the University of Bochum at La Silla/Chile. Spectral fluxes of the program stars have been determined with an error of 0m.03 or less.

Type
III. The Circumstellar Gas
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 206 - 207
Copyright
Copyright © Cambridge University Press 1987

References

Barbier, D., Chalonge, D.: 1941, Ann. Astrophys. 4, 75 Google Scholar
Kaiser, D.: 1986, Astron. Astrophys. Suppl. Ser., in pressGoogle Scholar
Kurucz, R. L.: 1979, Astrophys. J. Suppl. 40, 1 CrossRefGoogle Scholar
Schild, R. E.: 1978, Astrophys. J. Suppl. 37, 77 CrossRefGoogle Scholar