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Continuum flux and polarization in B[e] supergiants
Published online by Cambridge University Press: 26 May 2016
Extract
B[e] supergiants constitute one group of stars in the upper left part of the HR diagram. On the basis of their hybrid spectrum and their intrinsic polarization a two components envelope was suggested (Zickgraf & Schulte-Ladbeck, 1989): a “polar wind” and a denser “equatorial disc”.
- Type
- 7. OB Stellar Winds
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- Copyright © Kluwer 1994