The KBSS-KCWI Survey: The connection between extended Ly halos and galaxy azimuthal angle at
arXiv:2104.10173 · doi:10.1093/mnras/stab2383
Abstract
We present the first statistical analysis of kinematically-resolved, spatially-extended Ly emission around galaxies in the Keck Baryonic Structure Survey (KBSS) using the Keck Cosmic Web Imager (KCWI). Our sample of 59 star-forming galaxies () comprises the subset with typical KCWI integration times of ~5 hours and with existing imaging data from the Hubble Space Telescope and/or adaptive optics-assisted integral field spectroscopy. The high resolution images were used to evaluate the azimuthal dependence of the diffuse Ly emission with respect to the stellar continuum within projected galactocentric distances of proper kpc. We introduce cylindrically-projected 2D spectra (CP2D) that map the averaged Ly spectral profile over a specified range of azimuthal angle, as a function of impact parameter around galaxies. The averaged CP2D spectrum of all galaxies shows clear signatures of Ly resonant scattering by outflowing gas. We stacked the CP2D spectra of individual galaxies over ranges of azimuthal angle with respect to their major axes. The extended Ly emission along the galaxy principal axes are statistically indistinguishable, with residual asymmetry of 2% () of the integrated Ly emission. The symmetry implies that the Ly scattering medium is dominated by outflows in all directions within 30 kpc. Meanwhile, we find that the blueshifted component of Ly emission is marginally stronger along galaxy minor axes for galaxies with relatively weak Ly emission. We speculate that this weak directional dependence of Ly emission becomes discernible only when the Ly escape fraction is low. These discoveries highlight the need for similar analyses in simulations with Ly radiative transfer modeling.
arXiv comment25 pages, 24 figures, 2 tables, accepted by MNRAS
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