Highly ejective feedback models under-predict X-ray luminosity of galaxy groups at fixed mass by 5.7 sigma using direct observables from 44 XMM-Newton observed systems.
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The impact of strong feedback on galaxy group scaling relations
Highly ejective feedback models under-predict X-ray luminosity of galaxy groups at fixed mass by 5.7 sigma using direct observables from 44 XMM-Newton observed systems.