Published September 1983 | Version v1
Journal article Metadata-only

A study of the binary system 58 Persei

Creators

  • 1. Royal Greenwich Observatory, Hailsham (UK)
  • 2. Sussex Univ., Brighton (UK)

Description

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. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
204
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
927-934
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
15019862
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
BINARY STARS; EXPERIMENTAL DATA; MAIN SEQUENCE STARS; SPECTROSCOPY; SUPERGIANT STARS; ULTRAVIOLET RADIATION; VISIBLE RADIATION
Descriptors DEC
DATA; ELECTROMAGNETIC RADIATION; GIANT STARS; INFORMATION; NUMERICAL DATA; RADIATIONS; STARS