Ionization-Gasdynamic Simulations of Wind-Blown Nebulae around Massive Stars
Using a code that employs a self-consistent method for computing the effects of photo-ionization on circumstellar gas dynamics, we model the formation of wind-driven nebulae around massive stars. We take into account changes in stellar properties and mass-loss over the star’s evolution. Our simulati...
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Format: | Article |
Language: | English |
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MDPI AG
2022-02-01
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Series: | Galaxies |
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Online Access: | https://www.mdpi.com/2075-4434/10/1/37 |