TY - GEN
T1 - Simulating radially outward winds within a turbulent gas clump
AU - Arreaga-García, Guillermo
AU - Topa, Silvio Oreste
PY - 2016/1/1
Y1 - 2016/1/1
N2 - © Springer International Publishing Switzerland 2016. By using the particle-based code Gadget2, we follow the evolution of a gas clump, in which a gravitational collapse is initially induced. The particles representing the gas clump have initially a velocity according to a turbulent spectrum built in a Fourier space of 643grid elements. In a very early stage of evolution of the clump, a set of gas particles representing the wind, suddenly move outwards from the clump’s center. We consider only two kinds of winds, namely: one with spherical symmetry and a second one being a bipolar collimated jet. In order to assess the dynamical change in the clump due to interaction with the winds, we show iso-velocity and iso-density plots for all our simulations.
AB - © Springer International Publishing Switzerland 2016. By using the particle-based code Gadget2, we follow the evolution of a gas clump, in which a gravitational collapse is initially induced. The particles representing the gas clump have initially a velocity according to a turbulent spectrum built in a Fourier space of 643grid elements. In a very early stage of evolution of the clump, a set of gas particles representing the wind, suddenly move outwards from the clump’s center. We consider only two kinds of winds, namely: one with spherical symmetry and a second one being a bipolar collimated jet. In order to assess the dynamical change in the clump due to interaction with the winds, we show iso-velocity and iso-density plots for all our simulations.
U2 - 10.1007/978-3-319-32243-8_23
DO - 10.1007/978-3-319-32243-8_23
M3 - Conference contribution
SN - 9783319322421
T3 - Communications in Computer and Information Science
SP - 326
EP - 342
BT - Simulating radially outward winds within a turbulent gas clump
T2 - Communications in Computer and Information Science
Y2 - 1 January 2016
ER -