Radiation hydrodynamic simulation of the Haro 11 galaxy : the escape of LyC and Lyα in a dwarf galaxy merger
(2026) In Monthly Notices of the Royal Astronomical Society 546(4).- Abstract
The Haro 11 galaxy merger is the closest known Lyman continuum (LyC) leaker and a strong Lyman-α (Lyα) emitter, making it an important analogue of the high-z galaxies that reionised the early Universe. To investigate how Haro 11’s properties arise, we perform a radiation hydrodynamics simulation of the merger, and create mock observations of LyC, Lyα, and Hα, from which we compute their luminosities (L) and escape fractions (fesc). We track these quantities along multiple sightlines as the two progenitor galaxies merge, from the first interaction until the system resembles the presentday Haro 11. We find that L and fesc vary by 1–2 orders of magnitude for LyC due to sightline variations. At the two pericentre... (More)
The Haro 11 galaxy merger is the closest known Lyman continuum (LyC) leaker and a strong Lyman-α (Lyα) emitter, making it an important analogue of the high-z galaxies that reionised the early Universe. To investigate how Haro 11’s properties arise, we perform a radiation hydrodynamics simulation of the merger, and create mock observations of LyC, Lyα, and Hα, from which we compute their luminosities (L) and escape fractions (fesc). We track these quantities along multiple sightlines as the two progenitor galaxies merge, from the first interaction until the system resembles the presentday Haro 11. We find that L and fesc vary by 1–2 orders of magnitude for LyC due to sightline variations. At the two pericentre passages, the total fLyCesc increases by roughly an order of magnitude. Conversely, fLyαesc shows a moderate increase at the pericentre passages, which affects the inference of LyC properties from Lyα. We attribute this to a displacement of the LyC-emitting stars relative to the Lyα-emitting gas, combined with an increased density from gas compression. Furthermore, fLyCesc is boosted during star formation bursts, likely due to stellar feedback. As direct comparison with Haro 11, the simulation qualitatively matches its morphology and luminosities. We find that among the dense stellar knots, knot C is the main contributor to both intrinsic and escaping LyC emission. Additionally, the Lyα spectra displays distinct features found in observations, implying similar gas conditions are present.
(Less)
- author
- Ejdetjärn, Timmy ; Östlin, Göran ; Rosdahl, Joakim ; Blaizot, Jérémy and Agertz, Oscar LU
- organization
- publishing date
- 2026-03-01
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- galaxies: evolution, galaxies: individual: Haro 11, galaxies: interactions, galaxies: star formation, galaxies: starburst, methods: numerical
- in
- Monthly Notices of the Royal Astronomical Society
- volume
- 546
- issue
- 4
- article number
- stag211
- publisher
- Oxford University Press
- external identifiers
-
- scopus:105030650347
- ISSN
- 0035-8711
- DOI
- 10.1093/mnras/stag211
- language
- English
- LU publication?
- yes
- id
- ab9f2f3c-a676-483d-8e57-6fea1878de17
- date added to LUP
- 2026-04-21 15:36:50
- date last changed
- 2026-04-21 15:37:39
@article{ab9f2f3c-a676-483d-8e57-6fea1878de17,
abstract = {{<p>The Haro 11 galaxy merger is the closest known Lyman continuum (LyC) leaker and a strong Lyman-α (Lyα) emitter, making it an important analogue of the high-z galaxies that reionised the early Universe. To investigate how Haro 11’s properties arise, we perform a radiation hydrodynamics simulation of the merger, and create mock observations of LyC, Lyα, and Hα, from which we compute their luminosities (L) and escape fractions (f<sub>esc</sub>). We track these quantities along multiple sightlines as the two progenitor galaxies merge, from the first interaction until the system resembles the presentday Haro 11. We find that L and f<sub>esc</sub> vary by 1–2 orders of magnitude for LyC due to sightline variations. At the two pericentre passages, the total f<sup>LyC</sup><sub>esc</sub> increases by roughly an order of magnitude. Conversely, f<sup>Lyα</sup><sub>esc</sub> shows a moderate increase at the pericentre passages, which affects the inference of LyC properties from Lyα. We attribute this to a displacement of the LyC-emitting stars relative to the Lyα-emitting gas, combined with an increased density from gas compression. Furthermore, f<sup>LyC</sup><sub>esc</sub> is boosted during star formation bursts, likely due to stellar feedback. As direct comparison with Haro 11, the simulation qualitatively matches its morphology and luminosities. We find that among the dense stellar knots, knot C is the main contributor to both intrinsic and escaping LyC emission. Additionally, the Lyα spectra displays distinct features found in observations, implying similar gas conditions are present.</p>}},
author = {{Ejdetjärn, Timmy and Östlin, Göran and Rosdahl, Joakim and Blaizot, Jérémy and Agertz, Oscar}},
issn = {{0035-8711}},
keywords = {{galaxies: evolution; galaxies: individual: Haro 11; galaxies: interactions; galaxies: star formation; galaxies: starburst; methods: numerical}},
language = {{eng}},
month = {{03}},
number = {{4}},
publisher = {{Oxford University Press}},
series = {{Monthly Notices of the Royal Astronomical Society}},
title = {{Radiation hydrodynamic simulation of the Haro 11 galaxy : the escape of LyC and Lyα in a dwarf galaxy merger}},
url = {{http://dx.doi.org/10.1093/mnras/stag211}},
doi = {{10.1093/mnras/stag211}},
volume = {{546}},
year = {{2026}},
}