The physics of Lyman a escape from high-redshift galaxies

Aaron Smith, Xiangcheng Ma, Volker Bromm, Steven L. Finkelstein, Philip F. Hopkins, Claude Andre Faucher-Giguere, Dusan Keres

Research output: Contribution to journalArticlepeer-review

49 Scopus citations

Abstract

Lyman a (Lya) photons from ionizing sources and cooling radiation undergo a complex resonant scattering process that generates unique spectral signatures in high-redshift galaxies. We present a detailed Lya radiative transfer study of a cosmological zoom-in simulation from the Feedback In Realistic Environments (FIRE) project. We focus on the time, spatial, and angular properties of the Lya emission over a redshift range of z = 5-7, after escaping the galaxy and being transmitted through the intergalactic medium (IGM). Over this epoch, our target galaxy has an average stellar mass of M∗ 5 × 108 M∗. We find that many of the interesting features of the Lya line can be understood in terms of the galaxy's star formation history. The time variability, spatial morphology, and anisotropy of Lya properties are consistent with current observations. For example, the rest-frame equivalent width has an EWLya,0 > 20 Å duty cycle of 62 per cent with a non-negligible number of sightlines with > 100 Å, associated with outflowing regions of a starburst with greater coincident UV continuum absorption, as these conditions generate redder, narrower (or single-peaked) line profiles. The lowest equivalent widths correspond to cosmological filaments, which have little impact on UV continuum photons but efficiently trap Lya and produce bluer, broader lines with less transmission through the IGM. We also show that in dense self-shielding, low-metallicity filaments and satellites, Lya radiation pressure can be dynamically important. Finally, despite a significant reduction in surface brightness with increasing redshift, Lya detections and spectroscopy of high-z galaxies with the upcoming James Webb Space Telescope is feasible.

Original languageEnglish (US)
Pages (from-to)39-59
Number of pages21
JournalMonthly Notices of the Royal Astronomical Society
Volume484
Issue number1
DOIs
StatePublished - Mar 21 2019

Keywords

  • Galaxies: formation
  • Galaxies: high-redshift
  • Radiative transfer

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'The physics of Lyman a escape from high-redshift galaxies'. Together they form a unique fingerprint.

Cite this