IAU Symp. 212, Special session on "Recent advances in nebular diagnostics of hot star atmospheres" ---------------------------------------------------------------- Coordinators: Daniel Schaerer, Sally Oey, Paul Crowther Main topics: - the impact of stellar atmosphere models on nebular diagnostics, results from new line blanketed model atmospheres - benchmarks for stellar + nebular modeling: detailed analysis of well studied HII or giant regions providing strong constraints on stellar and nebular models - calibrations of stellar and abundance diagnostics - new results from recent observations (especially ISO) The main focus of the session will be on new line blanketed model atmospheres, and the modeling of simple, well constrained HII regions providing the best tests for combined stellar and photoionisation models. The aim of the latter is to discuss the methodology, successes and failures of models of the ionised ISM. The coordinators intend to publish a summary of the session in the proceedings of the symposium. Program (Sunday 23 june) ------------------------ 15:00 -- 15:10 Conti Comments on stellar effective temperatures 15:10 -- 15:20 Puls A New Spectral-Type/Teff Calibration for Hot Stars 15:20 -- 15:30 Martins Status of line blanketed O star model atmospheres (CMFGEN and WMBASIC models) 15:30 -- 15:40 Norris WR model atmospheres compared with HII regions 15:40 -- 15:55 Crowther Discussion - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 15:55 -- 16:05 Schaerer Testing O star model atmospheres with nebular modeling (ISO results) 16:05 -- 16:15 Bresolin Nebular diagnostics and stellar populations of HII regions 16:15 -- 16:25 Luridiana The robustness of nebular diagnostics: which, why and when 16:25 -- 16:35 Castellanos Metal-rich HII regions (diagnostisc and modeling) 16:35 -- 16:45 Beckman Density bounded regions and leakage 16:45 -- 17:00 Oey Discussion --> For further information contact Daniel Schaerer (schaerer@ast.obs-mip.fr). ----------------------------------------------------------------------