A study of the binary system 58 Persei.
Stickland, D. J.; Lloyd, C.; Pike, C. D.; Harmer, D. L.; Harmer, C. F. W.; Croft, D.
United Kingdom
Abstract
The spectroscopic (and astrometric) binary 58 Persei has been observed at optical wavelengths and with IUE. The system is shown to consist of a mid B-type main-sequence star and a late G-type supergiant at a distance of 320 pc.