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Spectroscopic studies of OB stars in the Magellanic Clouds with VLT-UVES
Published online by Cambridge University Press: 26 May 2016
Abstract
We present results from optical and ultraviolet analysis of nine LMC/SMC supergiants. Temperatures, mass-loss rates and CNO abundances are obtained using the non-LTE, line-blanketed model atmosphere code of Hillier & Miller (1998). In general, the derived temperatures are significantly lower than those determined from unblanketed, plane-parallel models.
- Type
- Part 1. Atmospheres of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003