000007356 001__ 7356
000007356 005__ 20250117131945.0
000007356 037__ $$aCTALK-2025-0035
000007356 100__ $$aPoniatowski, L.
000007356 245__ $$aRadiation hydrodynamics under extreme conditions
000007356 260__ $$c2024
000007356 269__ $$c2024-07-11
000007356 520__ $$aDescribing the dynamics of optically thick, accelerating media involves intricate interactions between gas and radiation. These effects are the main drivers in the outflows of various diverse classes of objects nearing or exceeding the Eddington limit. Prominent examples include Wolf-Rayet (WR) stars and Luminous Blue Variables (LBVs), distinguished by their continuous or eruptive optically thick winds. This presentation delves into the complexities of Radiation Hydrodynamics Under Extreme Conditions, aiming to address unresolved observational and theoretical challenges while attempting to offer some insights into potential solutions.
000007356 594__ $$aNO
000007356 6531_ $$aRadiation transfere
000007356 6531_ $$aRadiation hydrodynamics
000007356 6531_ $$aExtreme conditions
000007356 6531_ $$aMassive star outflows
000007356 6531_ $$aNumerical
000007356 773__ $$tFundamentals of Stellar Outflows: Celebrating and Amplifying the Scientific Life of Stan Owocki; Leuven
000007356 8560_ $$fluka.poniatowski@ksb-orb.be
000007356 85642 $$ahttps://fys.kuleuven.be/ster/events/conferences/2024/stanfest
000007356 906__ $$aInvited
000007356 980__ $$aCTALKINVI