Evolution of WR ring nebulae generated by a moving central star - II. The influence of the red supergiant bow shock

Details Evolution of WR ring nebulae generated by a moving central star - II. The influence of the red supergiant bow shock Evolution of WR ring nebulae generated by a moving central star - II. The influence of the red supergiant bow shock

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.277...53b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 277, Issue 1, pp. 53-69.

Astronomy and Astrophysics

Astronomy

26

Hydrodynamics, Instabilities, Stars: Wolf-Rayet, Ism: Bubbles

Scientific paper

We present detailed 2D simulations of the evolution of Wolf-Rayet ring nebulae expanding around stars which move through the interstellar medium. Attention is paid to a description of how the circumstellar matter is processed by the previous action of the stellar wind during the red supergiant phase. In particular, the radiative bow shock around the red supergiant star suffers strong dynamical instabilities whose development influences the evolution of the ring nebula. The models are compared with some observed ring nebulae.

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