On the Observed Diversity of Star Formation Efficiencies in Giant Molecular Clouds

Kearn Grisdale; Oscar Agertz; Florent Renaud; Alessandro B. Romeo; Julien Devriendt; Adrianne Slyz

doi:10.1093/mnras/stz1201

paper

On the Observed Diversity of Star Formation Efficiencies in Giant Molecular Clouds

arXiv:1902.00518 · doi:10.1093/mnras/stz1201

Abstract

Observations find a median star formation efficiency per free-fall time in Milky Way Giant Molecular Clouds (GMCs) on the order of $ε_{ff} \sim 1%$ with dispersions of $\sim 0.5 dex$ . The origin of this scatter in $ε_{ff}$ is still debated and difficult to reproduce with analytical models. We track the formation, evolution and destruction of GMCs in a hydrodynamical simulation of a Milky Way-like galaxy and by deriving cloud properties in an observationally motivated way, measure the distribution of star formation efficiencies which are in excellent agreement with observations. We find no significant link between $ε_{ff}$ and any measured global property of GMCs (e.g. gas mass, velocity dispersion). Instead, a wide range of efficiencies exist in the entire parameter space. From the cloud evolutionary tracks, we find that each cloud follow a \emph{unique} evolutionary path which gives rise to wide diversity in all properties. We argue that it is this diversity in cloud properties, above all else, that results in the dispersion of $ε_{ff}$ .

arXiv comment10 pages, 6 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society

On the Observed Diversity of Star Formation Efficiencies in Giant Molecular Clouds

Abstract

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