SIMBAD references

1999A&A...344..199B - Astronomy and Astrophysics, volume 344199-204 (1999/4-1)

Optically thick super-Eddington winds in Galactic superluminal sources.

BELYANIN A.A.

Abstract (from CDS):

A model of major ejection events in Galactic superluminal sources GRO J 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.

Abstract Copyright: ∼

Journal keyword(s): acceleration of particles - accretion, accretion disks - radiation mechanisms: non-thermal - stars: individual: GRO J1655-40 - stars: individual: GRS 1915+105

Simbad objects: 3

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