Optically thick super-Eddington winds in Galactic superluminal sources Academic Article uri icon

abstract

  • A model of major ejection events in Galactic superluminal sources GROJ 1655-40 and GRS 1915-105 is proposed, in which episodes of e-e+pair creation give rise to the formation of optically thick outflows accelerating protons to the limiting Lorentz factor of order 2-3. Probable source of e-e+pairs is pion production in nucleon collisions. Subsequent deceleration of ejecta and formation of radio jets is analyzed in detail within a shock deceleration model. The detailed data available for GRO J 1655-40 are shown to be in good agreement with proposed scenario.

author list (cited authors)

  • Belyanin, A. A

complete list of authors

  • Belyanin, AA

publication date

  • January 1, 1999 11:11 AM