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Ultraviolet Spectrophotometry of Early-Type Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
The ultraviolet spectra of B stars obtained with the sky scan telescope in the TD1 satellite have been used to obtain narrow-band magnitudes at several wavelengths. These photometric bands have an effective half-width of 100 Å. We have proposed a two-dimensional classification scheme based on ultraviolet colours, and some preliminary results are presented.
- Type
- Part IV/Abundance Effects in Spectral Classification
- Information
- Symposium - International Astronomical Union , Volume 72: Abundance Effects in Classification , 1976 , pp. 161 - 165
- Copyright
- Copyright © Reidel 1976
References
- 3
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