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Quantitative spectroscopy of B supergiants in the Galaxy, the LMC and theSMC. I. The B0.5 IA supergiants kappa Orionis, SK -68 41 and SK 159.

D. J. Lennon, R. P. Kudritzki, Stefan Becker, K. Butler, F. Eber, Helen Groth, D. Kunze

Abstract

High resolution spectra of the B0.5 Ia supergiants κ Orionis, Sk-68°41 in the Large Magellanic Cloud (LMC) and Sk 159 in the Small Magellanic Cloud (SMC) are analysed using non-LTE model atmosphere and line formation calculations.

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Key concepts: Supergiant, Physics, Large Magellanic Cloud, Astrophysics, Blue supergiant, Galaxy, Astronomy, Small Magellanic Cloud