Possible representation for discovery observations of stellar flares

Details Possible representation for discovery observations of stellar flares Possible representation for discovery observations of stellar flares

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap.....38...11m&link_type=abstract

Astrophysics, Volume 38, Issue 1, pp.11-14

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is shown that the chronology of flare star discoveries in the Pleiades cluster and the Orion association can be described satisfactorily by various distribution functions (gamma, binomial, decreasing exponential, and delta) for the mean frequencies of stellar flares. However, it has been found that this is due to the uncertainty in the observationally derived distribution function for the mean frequency of stellar flares. The most likely function is that derived by Ambartsumian, which has a physical basis.

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