Radiatively Driven Winds of OB Stars -- from Micro to Macro

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dc.creatorKrticka, Jiri
dc.creatorKubat, Jiri
dc.date2005-11-15
dc.date.accessioned2026-07-07T06:45:07Z
dc.date.available2026-07-07T06:45:07Z
dc.descriptionWe review basic physics of line-driven stellar winds of OB stars. We discuss elementary processes due to which stellar winds are accelerated on a microscopic level. We show how these microscopic processes may enable the outflow and how they determine wind properties on a macroscopic level. We discuss shortcomings of present wind theories and future wind model improvements.
dc.description12 pages; to appear in the proceedings of Active OB-Stars: Laboratories for Stellar & Circumstellar Physics, S. Stefl, S. Owocki and A. Okazaki eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0511443
dc.identifierhttp://arxiv.org/abs/astro-ph/0511443
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102968
dc.subjectAstrophysics
dc.titleRadiatively Driven Winds of OB Stars -- from Micro to Macro
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