Discovery of a Damped Lyα Absorber Originating in a Spectacular Interacting Dwarf Galaxy Pair at z = 0.026 - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles The Astrophysical journal letters Year : 2022

Discovery of a Damped Lyα Absorber Originating in a Spectacular Interacting Dwarf Galaxy Pair at z = 0.026

Erin Boettcher
  • Function : Author
Neeraj Gupta
  • Function : Author
Hsiao-Wen Chen
  • Function : Author
Mandy C. Chen
  • Function : Author
Gyula I. G. Józsa
  • Function : Author
Gwen C. Rudie
  • Function : Author
Sebastiano Cantalupo
  • Function : Author
Sean D. Johnson
  • Function : Author
S. A. Balashev
  • Function : Author
Kathy L. Cooksey
  • Function : Author
Claude-André Faucher-Giguère
  • Function : Author
Jens-Kristian Krogager
  • Function : Author
Sebastian Lopez
  • Function : Author
Emmanuel Momjian
  • Function : Author
Marc Rafelski
  • Function : Author
Raghunathan Srianand
  • Function : Author
Gregory L. Walth
  • Function : Author
Fakhri S. Zahedy
  • Function : Author

Abstract

We present the discovery of neutral gas detected in both damped Lyα absorption (DLA) and H I 21 cm emission outside of the stellar body of a galaxy, the first such detection in the literature. A joint analysis between the Cosmic Ultraviolet Baryon Survey and the MeerKAT Absorption Line Survey reveals an H I bridge connecting two interacting dwarf galaxies (log (M star/M ) = 8.5 ± 0.2) that host a z = 0.026 DLA with log[N(H I)/cm-2] = 20.60 ± 0.05 toward the QSO J2339-5523 (z QSO = 1.35). At impact parameters of d = 6 and 33 kpc, the dwarf galaxies have no companions more luminous than ≍0.05L * within at least Δv = ±300 km s-1 and d ≍ 350 kpc. The H I 21 cm emission is spatially coincident with the DLA at the 2σ-3σ level per spectral channel over several adjacent beams. However, H I 21 cm absorption is not detected against the radio-bright QSO; if the background UV and radio sources are spatially aligned, the gas is either warm or clumpy (with a spin temperature to covering factor ratio T s /f c > 1880 K). Observations with VLT-MUSE demonstrate that the α-element abundance of the ionized interstellar medium (ISM) is consistent with the DLA (≍10% solar), suggesting that the neutral gas envelope is perturbed ISM gas. This study showcases the impact of dwarf-dwarf interactions on the physical and chemical state of neutral gas outside of star-forming regions. In the SKA era, joint UV and H I 21 cm analyses will be critical for connecting the cosmic neutral gas content to galaxy environments.
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insu-03717132 , version 1 (09-07-2022)

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Erin Boettcher, Neeraj Gupta, Hsiao-Wen Chen, Mandy C. Chen, Gyula I. G. Józsa, et al.. Discovery of a Damped Lyα Absorber Originating in a Spectacular Interacting Dwarf Galaxy Pair at z = 0.026. The Astrophysical journal letters, 2022, 926, ⟨10.3847/2041-8213/ac5250⟩. ⟨insu-03717132⟩
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