Jan 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..173p&link_type=abstract
Nature, vol. 253, Jan. 17, 1975, p. 173, 174.
Physics
23
Eclipsing Binary Stars, Emission Spectra, H Alpha Line, Stellar Mass Ejection, Stellar Spectra, Line Shape, Luminous Intensity, Mass Transfer, Stellar Atmospheres, Stellar Luminosity
Scientific paper
On August 8, 1974, very strong H-alpha emission from U Cephei during a primary eclipse was observed. The equipment available made it possible to study the behavior of the emission line in detail. The density tracings of nine consecutive spectrograms are presented in a graph and the peak intensities of the violet and red emission lobes as functions of phase are listed in a table.
Plavec Mirek
Polidan Ronald S.
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