Hard X-Ray Bursts from GRO J1744-128. II. Statistical Studies

Details Hard X-Ray Bursts from GRO J1744-128. II. Statistical Studies Hard X-Ray Bursts from GRO J1744-128. II. Statistical Studies

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...493..408a&link_type=abstract

Astrophysical Journal v.493, p.408

Astronomy and Astrophysics

Astronomy

Stars: Individual Alphanumeric: Gro J1744-28, Stars: Neutron, X-Rays: Bursts, X-Rays: Stars

Scientific paper

Statistical studies of the hard X-ray bursts from GRO J1744-28 observed by the Konus-Wind and Konus-A experiments are presented. It is shown that during the whole period of outburst activity, the intervals of time between successive bursts form a stochastic Markov sequence that is characterized by both the constancy of the mean interval and the existence of a weak negative correlation between two successive intervals. A weak correlation between burst strength and the adjacent intervals is also indicated.

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