The UV spectrum of the possible radio star HD 26676.
Bibcode: 1979A&A....77..359S
Stickland, D. J.
Spain
Abstract
Results are reported for low-resolution UV spectroscopy (1150-1950 A and 1850-3250 A) of the star HD 26676, which may be associated with a weak nonthermal radio source, from the IUE satellite. It is found that the energy distribution of this star appears to be that of a perfectly normal single B8 V star. It is concluded that HD 26676 is an unlikely candidate for a source of radio emission at this time.
1979
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Astronomy and Astrophysics
IUE
2