Abstract
The following conclusions support those drawn from statistical studies done by other authors:
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1.
The mean energy per flare increases with increasing intrinsic quiescent luminosity of the parent star.
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2.
Brighter flare stars have more energetic but less frequent flares.
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3.
The rise times become more rapid as the quiescent energy of the parent star decreases.
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4.
Most of the flare light curves are either combinations of spike and slow flares or successive overlapping flares, supporting the view that energy can be added at various times during the development and decay of a flare event.
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5.
Flares with greater energy release occasionally last longer.
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References
Bhatt T.R., Sinvhal S.D., 1971, IBVS 557
Bhatt T.R., Sinvhal S.D., 1971, IAU Coll. 15, 124
Cristaldi S., Rodono M., 1973, A&A Suppl. 10, 47
Kapoor R.C., Sinvhal S.D., 1972, IBVS 750
Kapoor R.C., 1973, IBVS 758
Kapoor R.C., Sanwal B.B., Sinvhal S.D., 1973, IBVS 810
Kapoor R.C., 1973, IBVS 848
Kapoor R.C., Sinvhal S.D., 1974, IBVS 901 Sanwal B.B., 1974, IBVS 932
Sanwal B.B., 1975, IBVS 998
Sanwal B.B., 1976, IBVS 1180
Sanwal B.B., 1976, IBVS 1210
Sanwal B.B., 1979, IBVS 1572
Sanwal B.B., 1982, IBVS 2143
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© 1995 Springer-Verlag
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Sanwal, B.B. (1995). Monitoring of flare stars at nainital observatory. In: Greiner, J., Duerbeck, H.W., Gershberg, R.E. (eds) Flares and Flashes. Lecture Notes in Physics, vol 454. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-60057-4_254
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DOI: https://doi.org/10.1007/3-540-60057-4_254
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