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Free keywords:
galaxies: evolution
galaxies: high redshift
galaxies: ISM
galaxies: star formation
galaxies: starburst
submillimetre: galaxies
Astrophysics - Astrophysics of Galaxies
Abstract:
We present ALMA Band 9 observations of the [C II]158 μm emission for a sample of 10 main-sequence galaxies at redshift z ̃ 2, with typical stellar masses (log M⋆/M☉ ̃ 10.0-10.9) and star formation rates (̃35-115 M☉ yr-1). Given the strong and well-understood evolution of the interstellar medium from the present to z = 2, we investigate the behaviour of the [C II] emission and empirically identify its primary driver. We detect [C II] from six galaxies (four secure and two tentative) and estimate ensemble averages including non-detections. The [C II]-to-infrared luminosity ratio ([C II]/LIR) of our sample is similar to that of local main- sequence galaxies (̃2 × 10-3), and ̃10 times higher than that of starbursts. The [C II] emission has an average spatial extent of 4-7 kpc, consistent with the optical size. Complementing our sample with literature data, we find that the [C II] luminosity correlates with galaxies' molecular gas mass, with a mean absolute deviation of 0.2 dex and without evident systematics: the [C II]-to-H2 conversion factor (α _[C II] ̃ 30 M☉/L☉) is largely independent of galaxies' depletion time, metallicity, and redshift. [C II] seems therefore a convenient tracer to estimate galaxies' molecular gas content regardless of their starburst or main-sequence nature, and extending to metal-poor galaxies at low and high redshifts. The dearth of [C II] emission reported for z > 6-7 galaxies might suggest either a high star formation efficiency or a small fraction of ultraviolet light from star formation reprocessed by dust.
