The distance to the Magellanic Clouds from luminous F supergiants.
A. Arellano Ferro, L. Mantegazza, E. Antonello
Abstract
A. Arellano Ferro, L. Mantegazza, E. Antonello
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
A significance statement is not available in the OpenAlex record.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
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