Light Curves of V711 Tauri (Hr 1099)

  • Il-Seong Nha
  • Joon-Young Oh


V and B observations of V711 Tauri (HR 1099) for the year 1982–1983 are presented. The light curves made with the data of this season are compared with those of the previous observations of the 1981–1982 season. The single-peaked maximum light had shifted slightly and the peak amplitude had decreased to 0.04 mag. in V. No clear sign of colour, BV, variation in comparison with the low temperature dark-spot is detected.


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  1. Blanco, C., Catalano, S., Marilli, E., Rodono, M., Scaltriti, F.: 1981, Inf. Bull. Var. Stars, No. 2000.Google Scholar
  2. Bopp, B. W., Fekel, F.: 1976, Astron. J. 81, 771.ADSCrossRefGoogle Scholar
  3. Cousins, A. W. J.: 1963, Monthly Notices Astron. Soc. S. Afr. 22, 58.ADSGoogle Scholar
  4. Dorren, J. D., Guinan, E. F.: 1982, Astrophys. J. 252, 296.ADSCrossRefGoogle Scholar
  5. Dorren, J. D., Siah, M. J., Guinan, E. F., McCook, G. P.: 1981, Astron. J. 86, 572.ADSCrossRefGoogle Scholar
  6. Mekkaden, M. V., Raveendran, A. V., Mohin, S.: 1982, J. Astrophys. Astron. 3, 27.ADSCrossRefGoogle Scholar
  7. Nha, I.-S., Kang: 1982, Publ. Astron. Soc. Pacific 94, 496.ADSCrossRefGoogle Scholar
  8. Nha, I.-S., Oh, J.-Y.: 1983, in ‘Activity in Red-Dwarf Stars’, IAU Colloq. 71, 409.Google Scholar
  9. Sarma, M. B. K., Ausekar, B. D., Prakasa Rao, B. V. N. S., Oh, J.-Y., Nha, I.-S.: 1985, Publ. Astron. Soc. Japan 37, 107.Google Scholar

Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • Il-Seong Nha
    • 1
  • Joon-Young Oh
    • 1
  1. 1.Yonsei University ObservatorySeoulKorea

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