Photon Bubbles in Young Massive Stars

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dc.creatorTurner, N. J.
dc.creatorYorke, H. W.
dc.creatorSocrates, A.
dc.creatorBlaes, O. M.
dc.date2004-03-31
dc.date.accessioned2026-07-07T07:42:12Z
dc.date.available2026-07-07T07:42:12Z
dc.descriptionSpectroscopic 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.
dc.description4 pages, 3 figures; to appear in "Gravitational Collapse: from Massive Stars to Planets", eds G. Garcia-Segura, G. Tenorio-Tagle, H. Yorke and J. Franco, Rev. Mex. A. A. S. C
dc.identifierhttps://arxiv.org/abs/astro-ph/0404004
dc.identifierhttp://arxiv.org/abs/astro-ph/0404004
dc.identifierRev.Mex.Astron.Astrofis. 22 (2004) 54-57
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122361
dc.subjectAstrophysics
dc.titlePhoton Bubbles in Young Massive Stars
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