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Numerics
AMR
-Self-Gravitational hydrodynamics with 3d AMR: methodolgy and applications to molecular cloud collapse and fragmentation. Truelove, Klein, Mc Kee, et al. (‘98)
Sink Particles
-Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPHFFedderath, et al. (‘10)
Self Similarity Solutions for Collapse
-Self-similar collapse of isothermal spheres and star formation Shu (‘77)
-The collapse of unstable isothermal spheres Hunter, (‘77)
-Dynamics of self-gravitating gaseous spheres-III. Analytical results in the free-fall of isothermal case Larson & Penston, et al. (‘04)
Bonnor Ebert Spheres
-"The formation and evolution of protostellar discs; three-dimensional adaptive mesh refinement hydrosimulations of collapsing, rotating Bonnor-Ebert spheres" Banerjee & Pudritz, et al. (‘04)
-"Gravitational Collapse of an Isothermal Sphere" Foster and Chevalier (‘93)
-"Protostellar collapse by compression" Hennebelle, Whitworth, Gladwin, Andre (‘2002)
Molecular Clouds
Turbulence
Stellar Feedback
Stellar feedback by radiation pressure and photoionization
Sales, Marinacci, Springel, Petkova, 2013