Deciphering Lyman-α Emission Deep into the Epoch of Reionisation
arxiv(2023)
摘要
During the epoch of reionisation the first galaxies were enshrouded in
pristine neutral gas, with one of the brightest emission lines in star-forming
galaxies, Lyman-α (Lyα), expected to remain undetected until the
Universe became ionised. Providing an explanation for the surprising detection
of Lyα in these early galaxies is a major challenge for extra-galactic
studies. Recent JWST observations have reignited the debate on whether
residence in an overdensity of galaxies is a it sufficient and necessary
condition for Lyα to escape. Here, we take unique advantage of both
high-resolution and high-sensitivity images from the JWST instrument NIRCam to
reveal that all galaxies in a sample of z>7 Lyα emitters have close
companions. We exploit novel on-the-fly radiative transfer
magnetohydrodynamical simulations with cosmic ray feedback to show that
galaxies with frequent mergers have very bursty star formation which drives
episodes of high intrinsic Lyα emission and facilitates the escape of
Lyα photons along channels cleared of neutral gas. We conclude that the
rapid build up of stellar mass through mergers presents a compelling solution
to the long-standing puzzle of the detection of Lyα emission deep into
the epoch of reionisation.
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