On the observed diversity of star formation efficiencies in Giant Molecular Clouds

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Abstract

Observations find a median star formation efficiency per free-fall time in Milky Way Giant Molecular Clouds (GMCs) of the order of ϵff∼1 per cent with dispersions of ∼0.5dex⁠. The origin of this scatter in ϵff 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, we measure the distribution of star formation efficiencies which are in excellent agreement with observations. We find no significant link between ϵff 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 follows a unique evolutionary path which gives rise to a wide diversity in all properties. We argue that it is this diversity in cloud properties, above everything else, that results in the dispersion of ϵff.

Detaljer

Författare
Enheter & grupper
Externa organisationer
  • University of Oxford
  • Chalmers University of Technology
Forskningsområden

Ämnesklassifikation (UKÄ) – OBLIGATORISK

  • Astronomi, astrofysik och kosmologi
  • Polymerkemi

Nyckelord

Originalspråkengelska
Sidor (från-till)5482-5491
Antal sidor10
Tidskriftmnras
Volym486
Utgivningsnummer4
StatusPublished - 2019 jul 1
PublikationskategoriForskning
Peer review utfördJa