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Disk Winds of B[e] Supergiants
DOI: 10.1007/BFb0106353
Bibcode: 1999LNP...523...40Z
Zickgraf, Franz-Josef
The class of B[e] supegiants is characterized by a two-component stellar wind consisting of a normal hot star wind in the polar zone and a slow and dense disk-like wind in the equatorial region. The properties of the disk wind are discussed using satellite UV spectra of stars seen edge-on, i.e. through the equatorial disk. These observations show …
1999
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IAU Colloq. 169: Variable and Non-spherical Stellar Winds in Luminous Hot Stars
IUE
8