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.
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Spectra of the western eROSITA bubbles reveal two uniform components at 0.60 keV and 0.21 keV with sub-solar abundances, plus a geometrical model constraining horizontal size to ~6 kpc but leaving vertical extent uncertain.
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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.
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The SRG/eROSITA diffuse soft X-ray background II. spectra and morphology of the eROSITA bubbles in the western Galactic hemisphere
Spectra of the western eROSITA bubbles reveal two uniform components at 0.60 keV and 0.21 keV with sub-solar abundances, plus a geometrical model constraining horizontal size to ~6 kpc but leaving vertical extent uncertain.