Spectroscopic investigation of the reaction of oxides with metallic surfaces I. Systems SiO2-Mo and SiO2-Kh18N9T steel

1971 ◽  
Vol 10 (12) ◽  
pp. 992-994
Author(s):  
D. M. Karpinos ◽  
S. P. Listovnichaya
1972 ◽  
Vol 11 (6) ◽  
pp. 484-487 ◽  
Author(s):  
D. M. Karpinos ◽  
S. P. Listovnichaya ◽  
V. Ya. Aivazov

1978 ◽  
Vol 17 (4) ◽  
pp. 296-299
Author(s):  
D. M. Karpinos ◽  
S. P. Listovnichaya ◽  
V. N. Balakhnina ◽  
Yu. N. Okunevskii ◽  
K. V. Rozanov

1965 ◽  
Vol 5 ◽  
pp. 120-130
Author(s):  
T. S. Galkina

It is necessary to have quantitative estimates of the intensity of lines (both absorption and emission) to obtain the physical parameters of the atmosphere of components.Some years ago at the Crimean observatory we began the spectroscopic investigation of close binary systems of the early spectral type with components WR, Of, O, B to try and obtain more quantitative information from the study of the spectra of the components.


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