The importance of radiative feedback for the stellar initial mass function
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Open Access
- 16 January 2009
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 392 (4) , 1363-1380
- https://doi.org/10.1111/j.1365-2966.2008.14165.x
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- Evidence for a Turnover in the Initial Mass Function of Low-Mass Stars and Substellar Objects: Analysis from an Ensemble of Young ClustersThe Astrophysical Journal, 2008
- The dependence of the initial mass function on metallicity and the opacity limit for fragmentationMonthly Notices of the Royal Astronomical Society, 2005
- The origin of the initial mass function and its dependence on the mean Jeans mass in molecular cloudsMonthly Notices of the Royal Astronomical Society, 2005
- The formation of a star cluster: predicting the properties of stars and brown dwarfsMonthly Notices of the Royal Astronomical Society, 2003
- The formation of close binary systems by dynamical interactions and orbital decayMonthly Notices of the Royal Astronomical Society, 2002
- The Formation and Fragmentation of Primordial Molecular CloudsThe Astrophysical Journal, 2000
- Resolution requirements for smoothed particle hydrodynamics calculations with self-gravityMonthly Notices of the Royal Astronomical Society, 1997
- A Theory of the Initial Mass Function for Star Formation in Molecular CloudsThe Astrophysical Journal, 1996
- Modelling accretion in protobinary systemsMonthly Notices of the Royal Astronomical Society, 1995
- Low-Temperature Rosseland Opacity TablesThe Astrophysical Journal Supplement Series, 1975