High energy radiation from the center of the local supercluster

Details High energy radiation from the center of the local supercluster High energy radiation from the center of the local supercluster

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aph.....6..387a&link_type=abstract

ASTROPARTICLE PHYSICS, Volume 6, Issue 3-4, p. 387-394.

Physics

2

Scientific paper

Evidence in X-rays, gamma rays and ultra high energy cosmic rays (UHCR) suggests the existence of active centers in extragalactic space which eject high energy particles and quanta. A concentration of these highest energy sources in the direction of the Local Supercluster indicates that the brightest apparent magnitude AGN's such as 3C274 (M87), 3C273, 3C279 and Markarian 421 are the only candidate sources for this radiation. A theoretical model of mass creation in the Local Supercluster based on a Machian theory of gravitation is described as a possible mechanism for production of the high energy while at the same time allowing the AGN's to be at the relatively close distance of the Supercluster. The fact that infrared photons fill intergalactic space limits the distance to the UHCR sources at a little over twice the distance to the center of the Local Supercluster strongly localizing the highest energy radiation to this relatively close distance.

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