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A Super-Eddington Wind Model for GRO J1655-40The 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.
Document ID
20060035298
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Meier, David L.
Date Acquired
August 23, 2013
Publication Date
July 15, 1997
Distribution Limits
Public
Copyright
Other
Keywords
Super-Eddington

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