XRISM/Resolve data on Mrk 509 show a tentative 3.6-sigma infalling absorber at 11000 km/s located within thousands of gravitational radii, interpreted as raining clumps from a failed wind.
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Experimental K-shell x-ray and EUV spectra from charge exchange collisions of Ar18+ and O8+ ions with neutrals in an EBIT, compared to multichannel Landau-Zener models.
citing papers explorer
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Is XRISM/Resolve probing a "raining" absorber in Mrk 509?
XRISM/Resolve data on Mrk 509 show a tentative 3.6-sigma infalling absorber at 11000 km/s located within thousands of gravitational radii, interpreted as raining clumps from a failed wind.
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X-ray and extreme-ultraviolet spectra from collisions of Ar$^{18+}$ and O$^{8+}$ ions with neutrals
Experimental K-shell x-ray and EUV spectra from charge exchange collisions of Ar18+ and O8+ ions with neutrals in an EBIT, compared to multichannel Landau-Zener models.