Version 75 (modified by 10 years ago) ( diff ) | ,
---|
Erica's Super Literature Library!
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
-Simulations of interstellar turbulence Elmegreen (2004)
-
Stellar Feedback
-Stellar feedback by radiation pressure and photoionization Sales, Marinacci, Springel, Petkova, 2013
Thermal Instability
-On the thermal instability in numerical models of the interstellar medium Dib, Burkert, Hujeirat
-Thermal instability in turbulent models of the ISM -Gazol, Semedani, Salcedo
Attachments (4)
- Hennebelle1.png (385.0 KB ) - added by 12 years ago.
- Hennebell2.jpg (371.7 KB ) - added by 12 years ago.
- Hennebelle1.jpg (383.1 KB ) - added by 12 years ago.
- Intro2ISM.pdf (1.4 MB ) - added by 10 years ago.