Abstract
The possible variation of the flare frequency of flare stars in the Orion association is considered. It is shown that of the 23 chosen stars, each having exhibited four or more flares, a change in flare frequency at the 0.1 significance level can be suspected for 13.
Similar content being viewed by others
REFERENCES
A. A. Akopian, Astrofizika, 42, 555 (1999).
A. A. Akopian, Astrofizika, 44, 131 (2001).
V. A. Ambartsumian, L. V. Mirzoyan, E. S. Parsamian, O. S. Chavushian, and L. K. Erastova, Astrofizika, 7, 319 (1971).
E. S. Parsamian and A. D. Andrews, Irish Astron. J., 23, No. 2, 183 (1996).
L. V. Mirzoyan and G. B. Ohanian, Astrofizika, 13, 561 (1977).
R. Sh. Natsvlishvili, Astrofizika, 34, 107 (1991).
E. Chavira and E. S. Parsamian, Rev. Mex. Astron. Astrofis., 22, 15 (1991).
E. S. Parsamian, E. Chavira, and G. Gonzalez, Rev. Mex. Astron. Astrofis., 25, 71 (1993).
N. D. Melikian and M. Della Valle, Inf. Bull. Var. Stars, No. 2929 (1986).
E. S. Parsamian, Inf. Bull. Var. Stars, No. 3498 (1990).
V. A. Ambartsumian, Astrofizika, 14, 367 (1978).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Akopian, A.A., Sargsyan, L.A. Variation in the Flare Frequency of Flare Stars. III. Flare Stars in the Orion Association. Astrophysics 45, 20–24 (2002). https://doi.org/10.1023/A:1015390424851
Issue Date:
DOI: https://doi.org/10.1023/A:1015390424851