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The distance to the Magellanic Clouds from luminous F supergiants.

A. Arellano Ferro, L. Mantegazza, E. Antonello

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Abstract

A recent M V −uvbyβ calibration for Galactic luminous F-G supergiants was used to estimate the distance to the Magellanic Clouds from F supergiants. The distance moduli 19.33 ± 0.31 for the SMC and 18.19 ± 0.22 for the LMC are found. The present limitations of using F-G supergiants at distance indicators are discussed

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What this paper is about

A recent M V −uvbyβ calibration for Galactic luminous F-G supergiants was used to estimate the distance to the Magellanic Clouds from F supergiants. The distance moduli 19.33 ± 0.31 for the SMC and 18.19 ± 0.22 for the LMC are found. The present limitations of using F-G supergiants at distance indicators are discussed

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Available abstract

A recent M V −uvbyβ calibration for Galactic luminous F-G supergiants was used to estimate the distance to the Magellanic Clouds from F supergiants. The distance moduli 19.33 ± 0.31 for the SMC and 18.19 ± 0.22 for the LMC are found. The present limitations of using F-G supergiants at distance indicators are discussed

Key concepts: Supergiant, Physics, Blue supergiant, Astrophysics, Astronomy, Large Magellanic Cloud, Distance modulus, Red supergiant

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