Abstract
RR TrA is an Algol-type eclipsing binary with a period of 0 d. 7131. The components are believed to be of spectral types B9 V and F0 IV. The analysis presented is based on previously unreduced observations made by Somerville in 1961–63. Orbital elements are obtained using the Wood model, and these indicate that the system is semi-detached, and that the eclipses are marginally complete. The components appear to be of unusually small size for their spectral classes. The solution presented is compared with earlier ones for this system obtained by Kwee and by Giuricin and Mardirossian, and similarities and differences between these solutions are noted.
Similar content being viewed by others
References
Al-Naimiy, H. A.: 1978,Astrophys. Space Sci. 53, 181.
Bok, B. J.: 1963,Quart. J. Roy. Astron. Soc. 4, 232.
Chambliss, C. R.: 1976,Publ. Astron. Soc. Pacific 88, 22.
Chambliss, C. R.: 1983,Astrophys. Space Sci. 89, 15.
FitzGerald, M. P.: 1970,Astron. Astrophys. 4, 234.
Giuricin, G. and Mardirossian, F.: 1981,Astron. Astrophys. Suppl. 45, 85.
Hoffleit, D.: 1931,Harvard Obs. Bull., No. 884.
Hoffmeister, C.: 1943,Kl. Veröff. Berlin-Babelsberg, No. 27.
Kwee, K. K., Oosterhoff, P. T., and Volders, L. M. J. S.: 1957,Bull. Astron. Inst. Neth. 13, 328.
Pickering, E. C.: 1910,Harvard Obs. Cir., No. 162.
Plavec, M. and Kratochvíl, P.: 1964,Bull. Astron. Inst. Czech. 15, 165.
Popper, D. M.: 1980,Ann. Rev. Astron. Astrophys. 18, 115.
Russell, H. N. and Merrill, J. E.: 1952,Contrib. Princeton Univ. Obs., No. 26.
Wood, D. B.: 1971,Astron. J. 76, 701.
Wood, D. B.: 1972, NASA Publ. X-110-72-473.
Wood, D. B. and Etzel, P. B.: 1982, private communication.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Chambliss, C.R. RR trianguli australis: A new analysis of a semi-detached system of unusually small dimensions. Astrophys Space Sci 104, 205–217 (1984). https://doi.org/10.1007/BF00650296
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650296