A study of the binary system 58 Persei

Details A study of the binary system 58 Persei A study of the binary system 58 Persei

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..927h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Sept. 1983, p. 927-934.

Astronomy and Astrophysics

Astronomy

3

B Stars, Binary Stars, Supergiant Stars, Ultraviolet Astronomy, G Stars, High Dispersion Spectrographs, Iue, Late Stars, Stellar Color, Stellar Evolution

Scientific paper

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.

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