The Winds and Disks of B[e] Supergiants

Details The Winds and Disks of B[e] Supergiants The Winds and Disks of B[e] Supergiants

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..185k&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

The problem of modeling the spectral energy distribution (SED) of B[e] supergiants (sgB[e]) is addressed. We suggest that the disks around sgB[e] are neutral in hydrogen at or close to the stellar surface, restricting the free-free (ff) and free-bound (fb) emission to the polar wind. Preliminary results for the LMC sgB[e] R 126 are in agreement with such a scenario and deliver a density contrast of ρequator/ρpole ≃ 120, typical for sgB[e].

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