Absence of nebular He{\sc ii} $\lambda$4686 constrains the UV emission from the Ultraluminous X-ray pulsar NGC~1313~X--2
While much has been learned in recent decades about the X-ray emission of the extragalactic Ultraluminous X-ray sources (ULXs), their radiative output in the UV band remains poorly constrained. Understanding of the full ULX spectral energy distribution (SED) is imperative to constrain the accretion...
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