Lyman continuum leaker candidates among highly ionised, low-redshift dwarf galaxies selected from He II

• Published in: Astronomy and astrophysics (Berlin) Vol. 672; p. A11
• Main Authors: Enders, A. U., Bomans, D. J., Wittje, A.
• Format: Journal Article
• Language: English
• Published: Heidelberg EDP Sciences 01.04.2023
• Subjects: Active galactic nuclei; Astronomy & Astrophysics; Compact galaxies; Constraints; Criteria; Dwarf galaxies; Emission analysis; Emitters; Helium isotopes; Intergalactic media; Interstellar matter; Ionization; Ionizing radiation; Metallicity; Photons; Radiation; Red shift; Spectroscopy; Star formation
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361/202245167

Context. Contemporary research suggests that the reionisation of the intergalactic medium (IGM) in the early Universe was predominantly realised by star-forming (proto-)galaxies (SFGs). Due to observational constraints, our knowledge on the origins of sufficient amounts of ionising Lyman continuum (LyC) photons and the mechanisms facilitating their transport into the IGM remains sparse. Recent efforts have thus focussed on the study of local analogues to these high-redshift objects. Aims. We aim to acquire a set of very low-redshift SFGs that exhibit signs of a hard radiation field being present. A subsequent analysis of their emission line properties is intended to shed light on how the conditions prevalent in these objects compare to those predicted to be present in early SFGs that are thought to be LyC emitters (LCEs). Methods. We used archival spectroscopic SDSS DR12 data to select a sample of low-redshift He  II 4686 emitters and restricted it to a set of SFGs with an emission line diagnostic sensitive to the presence of an active galactic nucleus, which serves as our only selection criterion. We performed a population spectral synthesis with FADO to reconstruct these galaxies’ star-formation histories (SFHs). Utilising the spectroscopic information at hand, we constrained the predominant ionisation mechanisms in these galaxies and inferred information on interstellar medium (ISM) conditions relevant for the escape of LyC radiation. Results. Our final sample consists of eighteen ionised, metal-poor galaxies (IMPs). These low-mass (6.2 ≤ log( M ⋆ / M ⊙ ) ≤ 8.8), low-metallicity (7.54 ≤ log(O/H) + 12 ≤ 8.13) dwarf galaxies appear to be predominantly ionised by stellar sources. We find large [O III] 5007/[O II] 3727 ratios and [S II] 6717,6731/H α deficiencies, which provide strong indications for these galaxies to be LCEs. At least 40% of these objects are candidates for featuring cosmologically significant LyC escape fractions ≳10%. The IMPs’ SFHs exhibit strong similarities and almost all galaxies appear to contain an old (> 1 Gyr) stellar component, while also harbouring a young, two-stage (∼10 Myr and < 1 Myr) starburst, which we speculate might be related to LyC escape. Conclusions. The properties of the compact emission line galaxies presented here align well with those observed in many local LCEs. In fact, our sample may prove as an extension to the rather small catalogue of local LCEs, as the extreme ISM conditions we find are assumed to facilitate LyC leakage. Notably, all of our eighteen candidates are significantly closer ( z  < 0.1) than most established LCEs. If the inferred LyC photon loss is genuine, this demonstrates that selecting SFGs from He  II 4686 is a powerful selection criterion in the search for LCEs.