Extremely high energy hadron and gamma-ray families(3). Core structure of the halo of superfamily

Details Extremely high energy hadron and gamma-ray families(3). Core structure of the halo of superfamily Extremely high energy hadron and gamma-ray families(3). Core structure of the halo of superfamily

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..368y&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 368-371 (SEE N85-35848 24-93)

Computer Science

Cosmic Rays, Electrons, Halos, Nuclear Interactions, Computer Techniques, Computerized Simulation, Correlation Coefficients, Nuclear Emulsions, Photometry

Scientific paper

The study of the core structure seen in the halo of Mini-Andromeda 3(M.A.3), which was observed in the Chacaltaya emulsion chamber, is presented. On the assumption that lateral distribution of darkness of the core is exponential type, i.e., D=D0exp(-R/r0), subtraction of D from halo darkness is performed until the cores are gone. The same quantity on cores obtained by this way are summarized. The analysis is preliminary and is going to be developed.

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