Add to ORKGThe authors report the results of the first computer simulations capable of following the condensation of protostars out of turbulent interstellar gases. These protostars are rotationally supported discs with masses in the range 2 - 20 Msun and diameters from 100 - 4000 AU. In many of the simulations multiple protostellar systems were formed
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...
The authors present numerical simulations illustrating two mechanisms of binary formation. In the fi...
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...
The authors report the results of the first computer simulations capable of following the condensati...
Attention is given to computer simulations of massive protostar formation which show that in regions...
We present numerical simulations of the formation of protostellar disks. The disks form in shocked l...
The authors report here computer simulations of protostars condensing out of interstellar gas. The s...
Numerical simulations of supersonic collisions between molecular subclouds and the resulting formati...
We investigate the formation of the first stars at the end of the cosmic dark ages with a suite of t...
Numerical simulations of protostars condensing out of turbulent interstellar gas clouds suggest that...
We investigate the collapse and fragmentation of low-mass, trans-sonically turbulent pre-stellar cor...
The formation of brown dwarfs (BDs) due to the fragmentation of early-stage protostellar discs under...
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...
The authors present numerical simulations illustrating two mechanisms of binary formation. In the fi...
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...
The authors report the results of the first computer simulations capable of following the condensati...
Attention is given to computer simulations of massive protostar formation which show that in regions...
We present numerical simulations of the formation of protostellar disks. The disks form in shocked l...
The authors report here computer simulations of protostars condensing out of interstellar gas. The s...
Numerical simulations of supersonic collisions between molecular subclouds and the resulting formati...
We investigate the formation of the first stars at the end of the cosmic dark ages with a suite of t...
Numerical simulations of protostars condensing out of turbulent interstellar gas clouds suggest that...
We investigate the collapse and fragmentation of low-mass, trans-sonically turbulent pre-stellar cor...
The formation of brown dwarfs (BDs) due to the fragmentation of early-stage protostellar discs under...
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...
The authors present numerical simulations illustrating two mechanisms of binary formation. In the fi...
It is expected that an average protostar will undergo at least one impulsive interaction with a neig...