X-ray luminous late-type giant binaries contribute ~20% of the GRXE continuum and ~40% of its iron line emission.
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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.
citing papers explorer
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X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission
X-ray luminous late-type giant binaries contribute ~20% of the GRXE continuum and ~40% of its iron line emission.
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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.