Tracing ionized gas kinematics in Lyman-break Analogs
Year: 2026
Type: article
Abstract: Context. The ionized gas kinematics of low-mass starburst galaxies is a tracer of galaxy interactions and feedback processes, which are key for understanding massive star formation, chemical enrichment, and galaxy evolution. Aims. We studied the ionized gas kinematics and outflow properties of a sample of Lyman-break analogs (LBAs) at z ∼ 0.1 − 0.3; these LBAs are characterized by compact morphologies, high UV luminosities, and strong emission lines, which are common at higher redshifts. Methods. We used high-resolution VLT/X-shooter spectra of 14 compact, UV-luminous LBAs to model the complex [O III ] λλ 4959,5007 Å and Balmer line profiles with multi-Gaussian fits. Results. The kinematics of LBAs are complex, with emission lines best reproduced by narrow ( σ < 90 km s −1 ) and broad ( σ > 90 km s −1 ) components in all galaxies. The narrow-line kinematics is highly turbulent, likely driven by massive star-forming clumps. The luminosities and line ratios of the narrow components are typical of giant H II regions. We interpret the broader components as ionized outflows driven by strong winds of massive stars and supernovae. In galaxies with highly complex profiles and disturbed morphologies, ongoing interactions or mergers are found to contribute to the broad components. We find outflow velocities ( v out ) in the range ∼200 km s −1 to 500 km s −1 . Simple models yield outflow mass rates of 0.20–2.72 M ⊙ yr −1 and mass-loading factors ( η ) of ∼0.03–0.81. We find that η shows a mild increasing trend at lower stellar masses, in agreement with previous observational studies and predictions from FIRE-2 and Illustris-TNG simulations. Compact starburst morphologies can modulate the η - M ★ relation, which is strongly correlated as Σ SFR - η , i.e., more compact starbursts drive stronger outflows. We find a good agreement with similar findings in star-forming galaxies at high redshifts ( z ∼ 2 − 9), including those from recent JWST observations. Conclusions. Our results highlight the relevance of detailed studies of the ionized gas kinematics in local UV-compact starbursts to improve our understanding of feedback processes in low-mass, rapidly star-forming galaxies.
Source: Astronomy and Astrophysics
Institutions: University of La Serena, Consejo Superior de Investigaciones Científicas, Centro de Estudios de Física del Cosmos de Aragón, Instituto de Astrofísica de Andalucía, Astronomical Observatory of Rome, National Institute for Astrophysics, Space Telescope Science Institute, University of Michigan
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $1,865
OpenAlex ID: W7118955634