Can planet formation resolve the dust budget crisis in high-redshift galaxies? (dataset)

  • Duncan Hugh Forgan (Creator)
  • K. Rowlands (Kate Elizabeth Rowlands) (Creator)
  • H. L. Gomez (Creator)
  • E. L. Gomez (Creator)
  • S. P. Schofield (Creator)
  • L. Dunne (Creator)
  • S. Maddox (S Maddox) (Creator)

Dataset

Description

This version of the code includes the planet formation process in the dust and metal evolution. This includes three new parameters (f_disc, f_wind, f_debris) which account for the fact that not all metals and dust are lost per unit star formation (classical astration) due to the planet formation process which can return some material back to the ISM.
Date made available11 Aug 2017
PublisherGitHub

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