Volume 605, September 2017
|Number of page(s)||19|
|Published online||11 September 2017|
Do galaxies that leak ionizing photons have extreme outflows?
1 Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290 Versoix, Switzerland
2 Astronomical Institute, Czech Academy of Sciences, Boční II 1401, 141 00 Prague, Czech Republic
3 CNRS, IRAP, 14 Avenue E. Belin, 31400 Toulouse, France
4 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
5 Main Astronomical Observatory, Ukrainian National Academy of Sciences, 27 Zabolotnoho str., 03143 Kyiv, Ukraine
6 Astronomy Department, University of Virginia, PO Box 400325, Charlottesville, VA 22904-4325, USA
Received: 13 February 2017
Accepted: 3 July 2017
Context. To reionize the early universe, high-energy photons must escape the galaxies that produce them. How these photons escape is debated because too many ionizing photons are absorbed even at small H i column densities. It has been suggested that stellar feedback drives galactic outflows out of star-forming regions, creating low density channels through which ionizing photons escape into the inter-galactic medium.
Aims. We compare the galactic outflow properties of confirmed Lyman continuum (LyC) leaking galaxies to a control sample of nearby star-forming galaxies to explore whether the outflows from leakers are extreme as compared to the control sample.
Methods. We use data from the Cosmic Origins Spectrograph on the Hubble Space Telescope to measure the equivalent widths and velocities of Si ii and Si iii absorption lines, tracing neutral and ionized galactic outflows. We explore whether the leakers have similar outflow properties to the control sample, and whether the outflows from the leakers follow similar scaling relations with host galaxy properties as the control sample. We rederive the escape fraction of ionizing photons for each leaker, and study whether the outflow properties influence the LyC escape fractions.
Results. We find that the Si ii and Si iii equivalent widths of the LyC leakers reside on the low-end of the trend established by the control sample. The leakers’ velocities are not statistically different than the control sample, but their absorption line profiles have a different asymmetry: their central velocities are closer to their maximum velocities. This possibly indicates a more rapidly accelerated outflow due to the compact size of the leakers. The outflow kinematics and equivalent widths are consistent with the scaling relations between outflow properties and host galaxy properties – most notably metallicity – defined by the control sample. Additionally, we use the Lyα profiles to show that the Si ii equivalent width scales with the Lyα peak velocity separation.
Conclusions. We determine that the low equivalent widths of the leakers are likely driven by low metallicities and low H i column densities, consistent with a density-bounded ionization region, although we cannot rule out significant variations in covering fraction. While we do not find that the LyC leakers have extreme outflow velocities, the low maximum-to-central velocity ratios demonstrate the importance of the acceleration and density profiles for LyC and Lyα escape.
Key words: galaxies: irregular / galaxies: ISM / galaxies: kinematics and dynamics / ISM: jets and outflows / galaxies: starburst
© ESO, 2017
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