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NLTE Line-Blanketed Model Stellar Atmospheres
Published online by Cambridge University Press: 26 May 2016
Abstract
We briefly review the assumptions and methods required to construct NLTE line-blanketed model atmospheres of hot stars. We describe our new grid of NLTE model atmospheres covering the parameter range of O stars at various metallicities. We have applied these new models to the analysis of HST/STIS and FUSE UV spectra of O stars in the SMC. This analysis leads us to revise down the effective temperature scale of O-type stars.
- Type
- Session B. Radiative Transfer
- Information
- Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 67 - 79
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
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