... reproduce the observed distribution of projected separations of pairs but predict that binary quasars are only observable as such in the early stages of galacticcollisions, after which the supermassive black holes would orbit within the merger remnant ...
... They further suggest that binary quasars ``are only observable as such in the early stages of galacticcollisions, after which the quiescent supermassive black holes orbit in the merger remnant for some time.' ...
... More importantly, because of the small CX cross sections at these high collision energies, CX line emission would be several orders of magnitude too weak to explain the Galactic plane emission. ...
... More importantly, because of the small CX cross sections at these high collision energies, CX line emission would be several orders of magnitude too weak to explain the Galactic plane emission. ...
... The Spectral Energy Distributions of Active Galactic Nuclei", . ... Active Galactic Nuclei", . ... STAR-DISK COLLISIONS AND THE ORIGIN OF BROAD LINES IN QUASARS" . ...
... When collisions occur between cosmic ray particles and atomic nuclei, gamma-rays are formed. Cosmic Rays . ... Image of the Trifid nebula . ACRONYMS . AGN . Active Galactic Nuclei . CV . ...
... Our results show, however, that even for these high Galactic latitude areas away from bright Galactic features, the line brightness varies significantly from field to field. ...
... The characteristic collision time for a binary is coll 0.8Gyr n5 a 100 v10 (Mbin + M ) (2) The total number of physical collisions (PCs) between RGs and NSs is NPC = nRG nNS RG,NS v , where nRG and nNS are the number densities of RGs and NSs accordingly ...
... 1991 The Einstein OGS Survey of Galactic Binary X-ray Sources (S.D. Vrtilek, J.E ... I. Collision Dominated Models (T.R. Kallman, S.D. Vrtilek, and S. Kahn), ApJ, 345 ...