Ultraviolet Spectrophotometry of Early-Type Stars
K. Nandy, G. I. Thompson, Colin M. Humphries
Abstract
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K. Nandy, G. I. Thompson, Colin M. Humphries
Abstract
Open-access reader
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.
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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.
Key concepts: Ultraviolet, Stars, Physics, Sky, Ultraviolet astronomy, Astrophysics, Telescope, Spectrophotometry