EDSER and Richardson-Lucy deconvolution of Chandra HETG zeroth-order images reveal a precessing two-knot structure in SS 433's jets, and PSF-subtracted spectra show no Fe lines in the outer regions, supporting non-thermal X-ray emission.
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Arcsecond-Scale X-ray Imaging and Spectroscopy of SS 433 with Chandra HETG
EDSER and Richardson-Lucy deconvolution of Chandra HETG zeroth-order images reveal a precessing two-knot structure in SS 433's jets, and PSF-subtracted spectra show no Fe lines in the outer regions, supporting non-thermal X-ray emission.