The UV spectrum of the possible radio star HD 26676

Details The UV spectrum of the possible radio star HD 26676 The UV spectrum of the possible radio star HD 26676

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....77..359s&link_type=abstract

Astronomy and Astrophysics, vol. 77, no. 3, Aug. 1979, p. 359, 360.

Astronomy and Astrophysics

Astrophysics

2

B Stars, Radio Stars, Ultraviolet Spectra, High Resolution, Iue, Nonthermal Radiation, Radio Emission

Scientific paper

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.

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