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 SPHF​Fedderath, 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