Projects per year
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 available | 11 Aug 2017 |
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Publisher | GitHub |
Projects
- 2 Finished
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Starting Grant - SEDmorph: Starting Grant 2012 SEDMorph
Wild, V. (PI)
1/09/12 → 31/01/18
Project: Standard
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ERC ECOGAL: Star Formation and the Galax: ECOGAL
Bonnell, I. A. (PI)
1/05/12 → 30/04/17
Project: Standard
Research output
- 1 Article
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Can planet formation resolve the dust budget crisis in high-redshift galaxies?
Forgan, D. H., Rowlands, K., Gomez, H. L., Gomez, E. L., Schofield, S. P., Dunne, L. & Maddox, S., Dec 2017, In: Monthly Notices of the Royal Astronomical Society. 472, 2, p. 2289-2296 8 p.Research output: Contribution to journal › Article › peer-review
Open AccessFile