NASA NTRS · 20060035298
A Super-Eddington Wind Model for GRO J1655-40
Abstract
The wind is responsible for determining the luminosity and spectral evolution of the object and for suppressing the formation of a fast, relativistic jet while the accretion rate is above the Eddington limit.
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Meier, David L.. 1997-07-15. A Super-Eddington Wind Model for GRO J1655-40. https://ntrs.nasa.gov/citations/20060035298
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