Photoelectric spectrophotometry of Wolf-Rayet stars

Details Photoelectric spectrophotometry of Wolf-Rayet stars Photoelectric spectrophotometry of Wolf-Rayet stars

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.170..611b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 170, Mar. 1975, p. 611-618.

Astronomy and Astrophysics

Astronomy

9

Emission Spectra, Hot Stars, Periodic Variations, Stellar Luminosity, Stellar Spectrophotometry, Wolf-Rayet Stars, Binary Stars, Diurnal Variations, Electrophotometry, Light (Visible Radiation), Line Shape, Luminous Intensity, Spectral Line Width, Variable Stars

Scientific paper

Photoelectric spectrum scans of five southern Wolf-Rayet stars in the spectral range 4600-4720 A were analyzed to study the variability of brightness and of emission line strengths. No variations of any kind in short time scale were found. However, in WC stars night-to-night variations of 3 to 4 per cent were detected in the emission line strengths.

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