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    • The Cool Accretion Disk in ESO 243-49 HLX-1: Further Evidence of an Intermediate-Mass Black Hole 

      Davis, Shane W.; Narayan, Ramesh; Zhu, Yucong; Barret, Didier; Farrell, Sean A.; Godet, Olivier; Servillat, Mathieu; Webb, Natalie A. (IOP Publishing, 2011)
      With an inferred bolometric luminosity exceeding \(10^{42}\;erg\;s^{–1}\), HLX-1 in ESO 243-49 is the most luminous of ultraluminous X-ray sources and provides one of the strongest cases for the existence of intermediate-mass ...