Lyman-alpha emission properties of simulated galaxies: interstellar medium structure and inclination effects
arXiv:1208.4781 · doi:10.1051/0004-6361/201218783
Abstract
[abridged] Aims. The aim of this paper is to assess the impact of the interstellar medium (ISM) physics on Lyman-alpha (Lya) radiation transfer and to quantify how galaxy orientation with respect to the line of sight alters observational signatures. Methods. We compare the results of Lya radiation transfer calculations through the ISM of a couple of idealized galaxy simulations with different ISM models. Results. First, the small-scale structuration of the ISM plays a determinant role in shaping a galaxys Lya properties.The artificially warm, and hence smooth, ISM of G1 yields an escape fraction of 50 percent at the Lya line center, and produces symmetrical double-peak profiles. On the contrary, in G2, most young stars are embedded in thick star-forming clouds, and the result is a 10 times lower escape fraction. G2 also displays a stronger outflowing velocity field, which favors the escape of red-shifted photons, resulting in an asymmetric Lya line. Second, the Lya properties of G2 strongly depend on the inclination at which it is observed: From edge-on to face-on, the line goes from a double-peak profile with an equivalent width of -5 Angstrom to a 15 times more luminous red-shifted asymmetric line with EW 90 Angstrom. Conclusions. Lya radiation transfer calculations can only lead to realistic properties in simulations where galaxies are resolved into giant molecular clouds, putting these calculations out of reach of current large scale cosmological simulations. Finally, we find inclination effects to be much stronger for Lya photons than for continuum radiation. This could potentially introduce severe biases in the selection function of narrow-band Lya emitter surveys, which could indeed miss a significant fraction of the high-z galaxy population.
13 pages, 11 figures, accepted for publication in Astronomy&Astrophysics
References in corpus (11)
- Slow Star Formation in Dense Gas: Evidence and Implications
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- 3D Lyman-alpha radiation transfer. I. Understanding Lyman-alpha line profile morphologies
- On the onset of galactic winds in quiescent star forming galaxies
- A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
- Where are the ``Missing'' Galactic Baryons?
- Lyman alpha Resonant Scattering in Young Galaxies - Predictions from Cosmological Simulations
- Lyman alpha emission in high-redshift galaxies
- The Polarization of Scattered Lyman Alpha Radiation Around High-Redshift Galaxies
- Signatures of reionization on Lyman alpha emitters
- The clustering of Ly-alpha emitters in a LambdaCDM Universe
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