Green Pea Galaxies Reveal Secrets of Ly Escape
arXiv:1506.02885 · doi:10.3847/0004-637X/820/2/130
Abstract
We analyze archival Ly spectra of 12 "Green Pea" galaxies observed with the Hubble Space Telescope, model their Ly profiles with radiative transfer models, and explore the dependence of Ly escape fraction on various properties. Green Pea galaxies are nearby compact starburst galaxies with [OIII]5007 equivalent widths of hundreds of Å. All 12 Green Pea galaxies in our sample show Ly lines in emission, with a Ly equivalent width distribution similar to high redshift Ly emitters. Combining the optical and UV spectra of Green Pea galaxies, we estimate their Ly escape fractions and find correlations between Ly escape fraction and kinematic features of Ly profiles. The escape fraction of Ly in these galaxies ranges from 1.4% to 67%. We also find that the Ly escape fraction depends strongly on metallicity and moderately on dust extinction. We compare their high-quality Ly profiles with single HI shell radiative transfer models and find that the Ly escape fraction anti-correlates with the derived HI column densities. Single shell models fit most Ly profiles well, but not the ones with highest escape fractions of Ly. Our results suggest that low HI column density and low metallicity are essential for Ly escape, and make a galaxy a Ly emitter.
arXiv comment9 figures, ApJ accepted
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