Hydrodynamical simulations of Pinwheel nebula WR 104

Details Hydrodynamical simulations of Pinwheel nebula WR 104 Hydrodynamical simulations of Pinwheel nebula WR 104

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..402l&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

1

Hydrodynamics, Methods: Numerical, Stars: Individual (Wr 104), Binaries, Stars: Winds, Outflows

Scientific paper

Pinwheel Nebulae are colliding wind binaries (CWB) composed of a Wolf-Rayet star and an early-type star. We first compare our simulations to analytic solutions for CWB. Then we perform large scale 2D simulations of the particular system WR 104. We determine the properties of the gas in the winds and confirm the flow in the spiral has a ballistic motion.

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