2020A&A...639A..85G -
Astronomy and Astrophysics, volume 639A85-85 (2020/7-1)
The origin of the escape of Lyman α and ionizing photons in Lyman continuum emitters.
GAZAGNES S., CHISHOLM J., SCHAERER D., VERHAMME A. and IZOTOV Y.
Abstract (from CDS):
Context.Identifying the physical mechanisms driving the escape of Lyman continuum (LyC) photons is crucial for the search of Lyman continuum emitter (LCE) candidates.
Aims. To understand the physical properties involved in the leakage of LyC photons, we investigate the connection between the HI covering fraction, HI velocity width, the Lyman α (Lyα) properties, and the escape of LyC photons in a sample of 22 star-forming galaxies, which includes 13 confirmed LCEs.
Methods. We fit the stellar continuum, dust attenuation, and absorption lines between 920Å and 1300Å to extract the HI covering fractions and dust attenuation. Additionally, we measure the HI velocity widths of the optically thick Lyman series and derive the Lyα equivalent widths (EW), escape fractions (fesc), peak velocities, and fluxes at the minimum of the observed Lyα profiles.
Results. Overall, we highlight strong observational correlations between the presence of low HI covering fractions and the observation of (1) low Lyα peak velocities; (2) more flux at the profile minimum; and (3) larger EW(Lyα), fesc(Lyα), and fescobs(LyC). Hence, low column density channels are crucialISM ingredients for the leakage of Lyα and LyC photons. Additionally, galaxies with narrower HI absorption velocity widths have higher Lyα equivalent widths, larger Lyα escape fractions, and lower Lyα peak velocity separations. This may suggest that these galaxies have low HI column density. Finally, we find that dust also regulates the amount of Lyα and LyC radiation that actually escapes theISM.
Conclusions. TheISM porosity is one of the origins of strong Lyα emission, enabling the escape of ionizing photons in low-z leakers. However, this is not sufficient to explain the largest fescobs(LyC), which indicates that the most extreme LCEs are likely to be density-bounded along all lines of sight to the observer. Overall, the neutral gas porosity provides a constraint for a lower limit to the escape fraction of LyC and Lyα photons, which offers a key estimator for assessing the leakage of ionizing photons.
Abstract Copyright:
© ESO 2020
Journal keyword(s):
dark ages, reionization, first stars - galaxies: ISM - ultraviolet: ISM - ISM: abundances - ISM: lines and bands - dust, extinction
Simbad objects:
26
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