Journal article
The new semi-analytic code GalICS 2.0 – reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously
- Abstract:
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GalICS 2.0 is a new semianalytic code to model the formation and evolution of galaxies in a cosmological context. N-body simulations based on a Planck cosmology are used to construct halo merger trees, track subhaloes, compute spins and measure concentrations. The accretion of gas onto galaxies and the morphological evolution of galaxies are modelled with prescriptions derived from hydrodynamic simulations. Star formation and stellar feedback are described with phenomenologi...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Accepted manuscript, pdf, 2.1MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stx1597
Authors
Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Issue:
- 2
- Publication date:
- 2017-07-14
- Acceptance date:
- 2017-06-22
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Keywords:
- Pubs id:
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pubs:702637
- UUID:
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uuid:d22bc66a-f60f-493f-8c29-7c8e9a1c8239
- Local pid:
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pubs:702637
- Source identifiers:
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702637
- Deposit date:
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2017-10-10
Terms of use
- Copyright holder:
- Cattaneo et al
- Copyright date:
- 2017
- Notes:
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This is the author accepted manuscript following peer review version of the article. The final version is
available online from Oxford University Press (OUP) at: https://doi.org/10.1093/mnras/stx1597
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