Radiation-hydrodynamic simulations of the formation of Orion-like star clusters. I. Implications for the origin of the initial mass function

Citation

Krumholz, M, Klein, R & McKee, C 2011, 'Radiation-hydrodynamic simulations of the formation of Orion-like star clusters. I. Implications for the origin of the initial mass function', The Astrophysical Journal, vol. 740, no. 2, pp. 1-16.

Year

2011

ANU Authors

Fields of Research

  • Cosmology And Extragalactic Astronomy
  • Galactic Astronomy

Updated:  29 May 2023 / Responsible Officer:  Director (Research Services Division) / Page Contact:  Researchers