Abstract
Long-period RS CVn-type binary CQ Aur was observed in 1987 and 1988.B andV light curves for the 1987 and 1988 epochs have been analyzed for the photometric solution by the modified Wilson and Devinney computing code with adjustable spot parameters. One-spot fit is good enough for the 1987 epoch while a wider distribution of spots in longitude is required for the 1988 epoch. The spot covers approximately 3% of total surface area of the cooler component. Absolute dimensions were deduced by combining Popper's spectroscopic results. The volume of the cooler component is approximately 100 times larger than that of the hotter component. Both components are subgiants but the cooler component evolved more than the hotter component.
Similar content being viewed by others
References
Busso, M., Scaltriti, F., Blanco, C., Catalano, S., Marilli, E., Pazzani, V., and Rodonó, M.: 1984,Astron. Astrophys. 135, 255.
Cerruti-Sola, M., Scaltriti, F., Blanco, C., Catalano, S., Marilli, F., Rodonó, M., Strazzula, G., and Chambliss, C. R.: 1980,Astron. Astrophys. Suppl. 42, 245.
Hall, D. S. and Kreiner, J. M.: 1980,Acta Astron. 30, 387.
Iben, I.: 1967,Ann. Rev. Astron. Astrophys. 5, 571.
Johnson, H. L. and Morgan, W. W.: 1953,Astrophys. J. 117, 313.
Kang, Y. W. and Wilson, R. E.: 1989,Astron. J. 97, 848.
O'Connell, D. J. K.: 1978,Ric. Astron. Specola Vatic. 8, 555.
Popper, D. M.: 1976,Inf. Bull. Var. Stars, No. 1083.
Popper, D. M.: 1990,Astron. J. 100, 247.
Scaltriti, F., Busso, M., and Cellino, A.: 1985,Inf. Bull. Var. Stars, No. 2841.
Svechnikov, M. A. and Bessonova, L. A.: 1984,CDS Bull., No. 26, 99.
Walter, F. M., Cash, W., Charles, P. A., and Bowyer, C. S.: 1980,Astrophys. J. 236, 212.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kang, Y.W. Photoelectric observations of long-period RS CVn binary CQ aurigae. Astrophys Space Sci 201, 35–45 (1993). https://doi.org/10.1007/BF00626971
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00626971