G. Polubek


This work presents a new solution for the close binary system DV Aqr (HD 199603, HR 8024) based on archival International Ultraviolet Explorer observations, ground-based photometric light curves and radial velocity data. The solution is obtained as the best t of the theoretical model to all these observations simultaneously. Roche geometry of the binary system is assumed and a grid of the newest Kurucz models of stellar atmospheres is used in the calculations.

Ключові слова

Stars; close binary; stars; individual; DV Aqr.

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