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DOI | 10.1093/MNRAS/STAA851 |
Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment | |
Hogarth L.; Amorín R.; Vílchez J.M.; Hägele G.F.; Cardaci M.; Pérez-Montero E.; Firpo V.; Jaskot A.; Chávez R. | |
发表日期 | 2020 |
ISSN | 358711 |
起始页码 | 3541 |
结束页码 | 3561 |
卷号 | 494期号:3 |
英文摘要 | We investigate the ionized gas kinematics, physical properties, and chemical abundances of Sloan Digital Sky Survey J142947, a Green Pea galaxy at redshift z ∼ 0.17 with strong, double-peak Ly α emission and indirect evidence of Lyman continuum (LyC) leakage. Using high-dispersion spectroscopy, we perform a multicomponent analysis of emission-line profiles. Our model consistently fits all lines as a narrow component with intrinsic velocity dispersion σ ∼ 40 km s-1, and two broader blue-shifted components with σ ∼ 90 and ∼250 km s-1. We find electron densities and temperatures, ionization conditions, and direct O/H and N/O abundances for each component. A highly ionized, metal-poor, young and compact starburst dominates narrow emission, showing evidence of hard radiation fields and elevated N/O. The blue-shifted broader components are consistent with highly turbulent, possibly clumpy ionized gas at the base of a strong photoionized outflow, which accounts for ≳50 per cent of the integrated emission-line fluxes. The outflow is dense and metal-enriched compared to the HII regions, with expansion velocities larger than those obtained from UV interstellar absorption lines under standard assumptions. Some of these metals may be able to escape, with outflows loading factors comparable to those found in high-z galaxies of similar SFR/Area. Our findings depict a two-stage starburst picture; hard radiation fields from young star clusters illuminate a turbulent and clumpy ISM that has been eroded by SNe feedback. Whilst UV data suggest an extended Ly α halo with high average HI column density, LyC photons could only escape from SDSS J142947 through low HI density channels or filaments in the ISM approaching density-bounded conditions, traced by outflowing gas. © 2020 The Author(s). |
英文关键词 | (cosmology:) reionization; Galaxies: abundances; Galaxies: dwarf; Galaxies: evolution; Galaxies: kinematics and dynamics; Galaxies: starburst |
来源期刊 | Monthly Notices of the Royal Astronomical Society |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/177041 |
作者单位 | University College London (UCL), London, WC1E 6BT, United Kingdom; Instituto de Investigacíon Multidisciplinar en Ciencia y Tecnologiá, Universidad de La Serena, Rául Bitrán 1305, La Serena, Chile; Departamento de Astronomiá, Universidad de La Serena, Av. Juan Cisternas 1200 Norte, La Serena, Chile; Instituto de Astrofísica de Andaluciá - CSIC, Glorieta de la Astronomiá s.n., Granada, E-18008, Spain; Instituto de Astrofísica de La Plata (UNLP - CONICET), La Plata, B1900FWA, Argentina; NSF's National Optical-Infrared Astronomy Research Laboratory, Gemini Observatory, Casilla 603, La Serena, Chile; Astronomy Department, Williams College, Williamstown, MA 01267, United States; CONACYT-Instituto de Radioastronomiá y Astrofísica, UNAM, Campus Morelia, Morelia, C.P. 58089, Mexico |
推荐引用方式 GB/T 7714 | Hogarth L.,Amorín R.,Vílchez J.M.,et al. Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment[J],2020,494(3). |
APA | Hogarth L..,Amorín R..,Vílchez J.M..,Hägele G.F..,Cardaci M..,...&Chávez R..(2020).Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment.Monthly Notices of the Royal Astronomical Society,494(3). |
MLA | Hogarth L.,et al."Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment".Monthly Notices of the Royal Astronomical Society 494.3(2020). |
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