Throughout the epoch of reionization the most luminous Ly{ \alpha} emitters are capable of ionizing their own local bubbles. The CR7 galaxy at $z \approx 6.6$ stands out for its combination of exceptionally bright Ly{ \alpha} and HeII 1640 Angstrom line emission but absence of metal lines. As a result CR7 may be the first viable candidate host of a young primordial starburst or direct collapse black hole. High-resolution spectroscopy reveals a +160 km s$^{ -1}$ velocity offset between the Ly{ \alpha} and HeII line peaks while the spatial extent of the Ly{ \alpha} emitting region is $\sim 16$ kpc. The observables are indicative of an outflow signature produced by a strong central source. We present one-dimensional radiation-hydrodynamics simulations incorporating accurate Ly{ \alpha} feedback and ionizing radiation to investigate the nature of the CR7 source. We find that a Population III star cluster with $10^5$ K blackbody emission ionizes its environment too efficiently to generate a significant velocity offset. However, a massive black hole with a nonthermal Compton-thick spectrum is able to reproduce the Ly{ \alpha} signatures as a result of higher photon trapping and longer potential lifetime. For both sources, Ly{ \alpha} radiation pressure turns out to be dynamically important.
Categories: astro-ph.GA