Photon Bubbles in Young Massive Stars
classification
🌌 astro-ph
keywords
starsyoungphotonanalysisbubblebubblescalculationsfields
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Spectroscopic studies indicate that gas in the photospheres of young O stars moves at speeds up to the sound speed. We show, using two-dimensional radiation MHD calculations and results from a local linear analysis, that the motions may be due to photon bubble instability if young O stars have magnetic fields.
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