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The Wind Momentum-Luminosity relationship: blue supergiants in the spiral galaxy NGC 300
Published online by Cambridge University Press: 26 May 2016
Abstract
We have carried out the wind analysis of six A-type supergiants in NGC 300. The derived Wind Momentum-Luminosity Relationship is compared with that of Galactic and M 31 blue supergiants and with theoretical models.
- Type
- Part 1. Atmospheres of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003