All simulations performed with the ORION code. Volume rendering produced with yt
STAR FORMING CLOUD
This movie shows a volume rendering of gas density; it zooms from large to small scales and ends with a forming protostar. The size appears in the bottom right corner.
Citation: Offner et al. 2009
PROTOSTELLAR OUTFLOW WITH MAGNETIC FIELDS
A volume rendering of the gas energy density (1/2 rho v2) for a simulated protostar launching an outflow. The box size is 0.26 pc.
Citation: Lee, Hull & Offner 2017, Image Credit: Neosha Narayanan
PROTOSTELLAR OUTFLOW: Density and Temperature
A volume rendering of both the gas density and temperature of a protostar launching an outflow. The temperature is computed using Hyperion. Box size is 800 AU.
Citation: Offner & Arce 2014, Robitaille 2011
TURBULENT ISOLATED CORE
Time evolution of the column density for 3 views of a simulated isolated dense core. A forming protostar launches an outflow that breaks out of the core. Box size is 0.26pc.
Citation: Offner & Arce 2014
PROTOSTELLAR OUTFLOW VELOCITY
Volume rendering showing the time evolution of the gas velocity. The protostar location is marked with a cross. Box size is 0.3pc.
FORMING STAR CLUSTER with RADIATION
Time evolution of projected column density (left) and temperature (right). Box size is 0.65 pc; time evolution is 0.15 Myr.