Abstract
Massive stars shape the surrounding ISM by emitting ionizing photons and ejecting material through stellar winds. We study the impact of the transfer of momentum from the wind of a massive star on the surrounding neutral or ionized material. We use the Smoothed Particle Hydrodynamics (SPH) code SEREN [3] including a newly implemented HEALPix-based momentum conserving wind scheme. The transfer of momentum from a wind onto the cold surrounding gas drives the expansion of a shock front, sweeping up the neutral material into a dense shell. In contrast, we find the momentum driven wind to have only little direct effect on the warm ionized gas.
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This project is funded by Deutsche Forschungsgesellschaft DFG PR 569/9-1
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Ngoumou, J., Hubber, D.A., Dale, J.E., Burkert, A. (2014). Effects of a Momentum Driven Stellar Wind on the Surrounding ISM. In: Stamatellos, D., Goodwin, S., Ward-Thompson, D. (eds) The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings, vol 36. Springer, Cham. https://doi.org/10.1007/978-3-319-03041-8_41
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DOI: https://doi.org/10.1007/978-3-319-03041-8_41
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