The [CII] emission as a molecular gas mass tracer in galaxies at low and high redshifts

A. Zanella, E. Daddi, G. Magdis, T. Diaz Santos, D. Cormier, D. Liu, A. Cibinel, R. Gobat, M. Dickinson, M. Sargent, G. Popping, S. C. Madden, M. Bethermin, T. M. Hughes, F. Valentino, W. Rujopakarn, M. Pannella, F. Bournaud, F. Walter, T. WangD. Elbaz, R. T. Coogan

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

89 Citas (Scopus)

Resumen

We present ALMA Band 9 observations of the [CII]158 μm emission for a sample of 10 mainsequence galaxies at redshift z ~ 2, with typical stellar masses (logM*/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 [CII] 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 (L[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 [CII] 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 [CII] luminosity correlates with galaxies' molecular gas mass, with a mean absolute deviation of 0.2 dex and without evident systematics: the [CII]- 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.

Idioma originalInglés
Páginas (desde-hasta)1976-1999
Número de páginas24
PublicaciónMonthly Notices of the Royal Astronomical Society
Volumen481
N.º2
DOI
EstadoPublicada - 1 dic. 2018
Publicado de forma externa

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