Abstract:
This paper reports on the results of a study of S59 ultraviolet spectral scans of the spectroscopic binaries β Persei, μ1 Scorpii and γ2 Velorum. In the case of μ1 Sco it was found that the Mg ii doublet at 2800 Å undergoes intensity variations that may be indicative of variable emission in the photographic spectrum. The continuum in the 2490-2590 Å range deviates from the continuum of the 'comparison stars'. In γ2 Vel, flux variations in the 2770-2870 Å region have been detected. © 1980 D. Reidel Publishing Co.
Referencias:
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Citas:
---------- APA ----------
Sahade, J. & Van der Hucht, K.A.
(1980)
. Ultraviolet observations of β Persei, μ1 Scorpii and γ2 Velorum with the TD-1A satellite. Astrophysics and Space Science, 69(2), 369-375.
http://dx.doi.org/10.1007/BF00661924---------- CHICAGO ----------
Sahade, J., Van der Hucht, K.A.
"Ultraviolet observations of β Persei, μ1 Scorpii and γ2 Velorum with the TD-1A satellite"
. Astrophysics and Space Science 69, no. 2
(1980) : 369-375.
http://dx.doi.org/10.1007/BF00661924---------- MLA ----------
Sahade, J., Van der Hucht, K.A.
"Ultraviolet observations of β Persei, μ1 Scorpii and γ2 Velorum with the TD-1A satellite"
. Astrophysics and Space Science, vol. 69, no. 2, 1980, pp. 369-375.
http://dx.doi.org/10.1007/BF00661924---------- VANCOUVER ----------
Sahade, J., Van der Hucht, K.A. Ultraviolet observations of β Persei, μ1 Scorpii and γ2 Velorum with the TD-1A satellite. Astrophys Space Sci. 1980;69(2):369-375.
http://dx.doi.org/10.1007/BF00661924