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Stellar winds in central stars of LMC planetary nebulae
Published online by Cambridge University Press: 15 December 2006
Abstract
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In this work we investigate the relation between wind momentum $\Pi$ and the luminosity of the CSPNs in the LMC taking advantage of the less uncertain distances to these objects. We show that these winds obey the same relation as the Galactic O stars and therefore have the same physics.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 359 - 360
- Copyright
- © 2006 International Astronomical Union
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