Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-09-28
Astron.Astrophys. 394 (2002) 901-910
Astronomy and Astrophysics
Astrophysics
9 pages, 3 figures, to be published in A&A
Scientific paper
10.1051/0004-6361:20021164
We study the dynamics of stellar wind bubbles around hydrogen-deficient stars using numerical simulations with time- and ion dependent cooling. We consider two types of hydrogen-deficient stars, massive WR stars, producing Ring Nebulae, and low mass [WR] stars, producing Planetary Nebulae. We show that for the Planetary Nebulae, the different cooling properties of the hydrogen-deficient wind lead to a later transition from momentum- to energy-driven flow, which could explain the observed turbulence of these nebulae. We find that Ring Nebulae should all be energy-driven, and show how comparing the bubble's momentum and kinetic energy to the input wind momentum and kinetic energy, can give misleading information about the dynamics of the bubble.
Lundqvist Peter
Mellema Garrelt
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