U, B, V photoelectric observations of the eclipsing binary system DX Aqr, secured in 1981, have been presented. Present results, when compared with earlier ones (cf. Srivastava and Sinha, 1985), suggest that the features of the system are changing. Some new features are reported.
This is a preview of subscription content, log in to check access.
We’re sorry, something doesn't seem to be working properly.
Please try refreshing the page. If that doesn't work, please contact support so we can address the problem.
Olsen, E. H.: 1976,Inf. Bull. Var. Stars, No. 1199.
Paffhausen, W. and Seggewiss, W.: 1976,Astron. Astrophys. Suppl. Ser. 24, 29.
Srivastava, R. K. and Sinha, B. K.: 1985,Astrophys. Space Science 111, 225.
Strohmeier W.: 1966,Inf. Bull. Var. Stars, No. 164.
About this article
Cite this article
Srivastava, R.K. Some observations of DX Aquarii. Astrophys Space Sci 113, 333–340 (1985). https://doi.org/10.1007/BF00650968
- Binary System
- Photoelectric Observation