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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Bibliographic Details
Main Author: Vikram V. Dwarkadas
Format: Article
Language:English
Published: MDPI AG 2022-02-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/10/1/37