Properties of five z ∼ 0.3-0.4 confirmed LyC leakers: VLT/XShooter observations - Archive ouverte HAL Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2020

Properties of five z ∼ 0.3-0.4 confirmed LyC leakers: VLT/XShooter observations

N. G. Guseva
  • Function : Author
Y. I. Izotov
  • Function : Author
J. M. Vílchez
  • Function : Author
R. Amorín
  • Function : Author
E. Pérez-Montero
  • Function : Author
J. Iglesias-Páramo
  • Function : Author
A. Verhamme
  • Function : Author
C. Kehrig
  • Function : Author


Using new Very Large Telescope (VLT)/XShooter spectral observations we analyse the physical properties of five z ~ 0.3-0.4 confirmed Lyman continuum (LyC) leakers. Strong resonant Mg II λλ2796, 2803 Å emission lines (I(λλ2796, 2803)/I(Hβ) ≃ 10-38 per cent) and non-resonant Fe II* λλ2612, 2626 Å emission lines are observed in spectra of five and three galaxies, respectively. We find high electron densities Ne ~ 400 cm-3, significantly higher than in typical low-z, but comparable to those measured in z ~ 2-3 star-forming galaxies (SFGs). The galaxies have a mean value of log N/O = -1.16, close to the maximum values found for SFGs in the metallicity range of 12 + log O/H ≃ 7.7-8.1. All 11 low-z LyC emitting galaxies found by Izotov et al., including the ones considered in this study, are characterized by high equivalent width (EW) (Hβ) ~ 200-400 Å, high ionization parameter (log(U) = -2.5 to -1.7), high average ionizing photon production efficiency ξ = 1025.54 Hz erg-1, and hard ionizing radiation. On the Baldwin-Phillips-Terlevich (BPT) diagram we find the same offset of our leakers from low-z main-sequence SFGs as that for local analogues of Lyman-break galaxies (LBGs) and extreme SFGs at z ~ 2-3. We confirm the effectiveness of the He I emission lines diagnostics proposed by Izotov et al. in searching for LyC leaker candidates and find that their intensity ratios correspond to those in a median with low neutral hydrogen column density N(H I) = 1017-5 × 1017 cm-2 that permit leakage of LyC radiation, likely due to their density-bounded H II regions.
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Dates and versions

insu-03673115 , version 1 (20-05-2022)



N. G. Guseva, Y. I. Izotov, D. Schaerer, J. M. Vílchez, R. Amorín, et al.. Properties of five z ∼ 0.3-0.4 confirmed LyC leakers: VLT/XShooter observations. Monthly Notices of the Royal Astronomical Society, 2020, 497, pp.4293-4310. ⟨10.1093/mnras/staa2197⟩. ⟨insu-03673115⟩
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