Ultraviolet observations of Beta Persei, MU super 1 Scorpii and Gamma2 Velorum with the TD-1A satellite

Details Ultraviolet observations of Beta Persei, MU super 1 Scorpii and Gamma2 Velorum with the TD-1A satellite Ultraviolet observations of Beta Persei, MU super 1 Scorpii and Gamma2 Velorum with the TD-1A satellite

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..369s&link_type=abstract

Astrophysics and Space Science, vol. 69, no. 2, May 1980, p. 369-375.

Astronomy and Astrophysics

Astronomy

Binary Stars, Line Spectra, Spaceborne Astronomy, Stellar Spectra, Td Satellites, Ultraviolet Astronomy, Emission Spectra, Magnesium, Radial Velocity, Satellite-Borne Instruments, Ultraviolet Spectra

Scientific paper

This paper reports on the results of a study of S59 ultraviolet spectral scans of the spectroscopic binaries Beta Persei, Mu super 1 Scorpii and Gamma2 Velorum. In the case of Mu super 1 Sco it was found that the Mg II doublet at 2800 A undergoes intensity variations that may be indicative of variable emission in the photographic spectrum. The continuum in the 2490-2590 A range deviates from the continuum of the comparison stars. In Gamma2 Vel, flux variations in the 2770-2870 A region have been detected.

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