2016MNRAS.460.3143S

Throughout the epoch of reionization, the most luminous Lyα emitters are capable of ionizing their own local bubbles. The CR7 galaxy at z ≃ 6.6 stands out for its combination of exceptionally bright Lyα and He ii 1640 Å 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 Lyα and He ii line peaks while the spatial extent of the Lyα emitting region is ∼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 Lyα 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 non-thermal Compton-thick spectrum is able to reproduce the Lyα signatures as a result of higher photon trapping and longer potential lifetime. For both sources, Lyα radiation pressure turns out to be dynamically important.