Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..181b&link_type=abstract
In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi
Astronomy and Astrophysics
Astronomy
46
Emission Spectra, Light Curve, Radial Velocity, Stellar Spectrophotometry, Ultraviolet Astronomy, Variable Stars, H Alpha Line, Power Spectra, Stellar Spectra
Scientific paper
Radial velocity observations of Lambda Eridani between 1971 and 1980 and uvbyH-alpha photometry in 1977 show that the star is both a light and velocity variable with a period of 0.701538 d. Copernicus observations in 1977 are compatible with this result. Both the radial velocity and photometric amplitude are variable, and these variations may be correlated with the hydrogen emission line strength. The character and phasing of the light and velocity curves suggest that Lambda Eridani is a pulsating variable.
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