A jet whose bulk Lorentz factor varies along its length, with the Doppler factor increasing outward, can naturally produce the soft self-absorbed radio spectra observed in many AGN and black-hole binaries.
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Variable jet Lorentz factors can explain soft self-absorbed radio spectra of accreting black-holes
A jet whose bulk Lorentz factor varies along its length, with the Doppler factor increasing outward, can naturally produce the soft self-absorbed radio spectra observed in many AGN and black-hole binaries.