Frequency distribution of x-ray flares for young stellar objects in the region of ρ Oph

Details Frequency distribution of x-ray flares for young stellar objects in the region of ρ Oph Frequency distribution of x-ray flares for young stellar objects in the region of ρ Oph

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap.....55...81a&link_type=abstract

Astrophysics, Volume 55, Issue 1, pp.81-91

Astronomy and Astrophysics

Astrophysics

X-Ray Flares, Frequency Distribution, Young Stellar Objects

Scientific paper

Methods for determining the frequency distribution function of optical flares have been developed and successfully applied in statistical studies of flare stars. X-ray observations of flare stars provide a basis for extending the use of these methods to statistical studies of X-ray flares of young stellar objects. This article gives a brief description of methods which can be used for determining the frequency distribution of the X-ray flares of young stellar objects. The corresponding function is determined for a sample of 195 low-mass young stellar objects in the cloud L1688, which forms part of the complex of dark clouds ρ Oph. It is found to have an exponential form.

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