Abstract
Photoelectric and absolute elements of the system RT Per have been determined inU, B, andV filters. It is suggested that the primary star may be surrounded by a gaseous disk.
Similar content being viewed by others
References
Batten, A. H.: 1973,Binary and Multiple System of Stars, Pergamon Press, p. 166.
Ceraski, L.: 1904,Astron. Nachr. 166, 155.
Chaubey, U. S.: 1979,Astrophys. Space Sci. 63, 247.
Chia, T. T.: 1977,Astrophys. Space Sci. 51, 33.
Dugan, R. S.: 1915,Monthly Notices Roy. Astron. Soc. 75, 692.
Grygar, J., Cooper, M. L., and Jurkevich, I.: 1972,Bull. Astron. Inst. Czech. 23, 147.
Guinan, E. F., Mc Cook, G. P., Bachmann, P. J., and Bistline, W. G.: 1976,Astron. J. 81, 57.
Hall, D. S. and Stuhlinger, T.: 1978,Acta Astron. 28, 207.
Hall, D. S. and Walker, K.: 1975,Astron. Astrophys. 38, 225.
Mancuso, S. and Milano, L.: 1975,AStrophys. Space Sci. 32, 385.
Mancuso, S. and Milano, L.: 1976,IAU Inf. Bull. Var. Stars, No. 1102.
Russell, H. N. and Merrill, J. E.: 1950,Princeton Univ. Contr., No. 23.
Russell, H. N. and Merrill J. E.: 1952,Princeton Univ. Contr., No. 26.
Struve, O.: 1947,Astrophys. J. 106, 92.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Sanwal, B.B., Chaubey, U.S. UBV photometry of RT Persei. Astrophys Space Sci 75, 329–340 (1981). https://doi.org/10.1007/BF00648646
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00648646