Ly$\alpha$ emission from Green Peas: the role of circumgalactic gas density, covering, and kinematics

TL;DR

This study uses Hubble observations of Green Pea galaxies to investigate how circumgalactic gas density, covering, and kinematics influence Ly$ extalpha$ emission and escape, revealing HI column density as a key regulator.

Contribution

It demonstrates that HI column density, not outflow velocity or covering fraction, primarily controls Ly$ extalpha$ escape in Green Pea galaxies.

Findings

Ly$ extalpha$ emission detected in all galaxies.

Ly$ extalpha$/H$ extalpha$ flux ratios indicate 5-60% photon escape.

Ly$ extalpha$ escape correlates with HI column density, not outflow velocity.

Abstract

We report Hubble Space Telescope/Cosmic Origins Spectrograph observations of the Ly$\alpha$ emission and interstellar absorption lines in a sample of ten star-forming galaxies at $z\sim0.2$. Selected on the basis of high equivalent width optical emission lines, the sample, dubbed "Green Peas," make some of the best analogs for young galaxies in an early Universe. We detect Ly$\alpha$ emission in all ten galaxies, and 9/10 show double-peaked line profiles suggestive of low HI column density. We measure Ly$\alpha$/H$\alpha$ flux ratios of 0.5-5.6, implying that 5% to 60% of Ly$\alpha$ photons escape the galaxies. These data confirm previous findings that low-ionization metal absorption (LIS) lines are weaker when Ly$\alpha$ escape fraction and equivalent width are higher. However, contrary to previously favored interpretations of this trend, increased Ly$\alpha$ output cannot be the result of varying HI covering: the Lyman absorption lines (Ly$\beta$ and higher) show a covering fraction near unity for gas with $N_{HI} \gtrsim 10^{16}$ cm$^{-2}$. Moreover, we detect no correlation between Ly$\alpha$ escape and the outflow velocity of the LIS lines, suggesting that kinematic effects do not explain the range of Ly$\alpha$/H$\alpha$ flux ratios in these galaxies. In contrast, we detect a strong anti-correlation between the Ly$\alpha$ escape fraction and the velocity separation of the Ly$\alpha$ emission peaks, driven primarily by the velocity of the blue peak. As this velocity separation is sensitive to HI column density, we conclude that Ly$\alpha$ escape in these Green Peas is likely regulated by the HI column density rather than outflow velocity or HI covering fraction.