XMM-Newton observations resolve three apparent low surface brightness galaxy groups into nine components, several with unusually flat X-ray surface brightness profiles, each with flux below previous RASS survey limits.
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XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
XMM-Newton observations resolve three apparent low surface brightness galaxy groups into nine components, several with unusually flat X-ray surface brightness profiles, each with flux below previous RASS survey limits.