On the power-law tail in the mass function of protostellar condensations and stars
- 21 January 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 347 (3)
- https://doi.org/10.1111/j.1365-2966.2004.07405.x
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This publication has 21 references indexed in Scilit:
- The formation of a star cluster: predicting the properties of stars and brown dwarfsMonthly Notices of the Royal Astronomical Society, 2003
- A Possible Origin of Lognormal Distributions in Gamma-Ray BurstsThe Astrophysical Journal, 2002
- A Fractal Origin for the Mass Spectrum of Interstellar Clouds. II. Cloud Models and Power‐Law SlopesThe Astrophysical Journal, 2002
- The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud FragmentationThe Astrophysical Journal, 2001
- Large‐Area Mapping at 850 Microns. II. Analysis of the Clump Distribution in the ρ Ophiuchi Molecular CloudThe Astrophysical Journal, 2000
- Mass segregation in young stellar clustersMonthly Notices of the Royal Astronomical Society, 1998
- On the Stellar Population and Star-Forming History of the Orion Nebula ClusterThe Astronomical Journal, 1997
- A Theory of the Initial Mass Function for Star Formation in Molecular CloudsThe Astrophysical Journal, 1996
- Boyle's Law and Gravitational InstabilityMonthly Notices of the Royal Astronomical Society, 1956
- On Spherically Symmetrical AccretionMonthly Notices of the Royal Astronomical Society, 1952