Ionization structure in the winds of B[e] supergiants
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065204/pdf
Reference37 articles.
1. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
2. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
3. Radiation-driven winds in Of stars
4. The Influence of Rotation in Radiation‐driven Wind from Hot Stars: New Solutions and Disk Formation in Be Stars
5. Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds
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1. Rings, Shells, and Arc Structures Around B[e] Supergiants. I. Classical Tools of Nonlinear Hydrodynamics;The Astrophysical Journal;2024-03-01
2. Discovering New B[e] Supergiants and Candidate Luminous Blue Variables in Nearby Galaxies;Galaxies;2023-06-19
3. A warm molecular ring in AG Car: composing the mass-loss puzzle;Monthly Notices of the Royal Astronomical Society;2020-11-20
4. A Census of B[e] Supergiants;Galaxies;2019-09-29
5. Resolving the kinematics of the discs around Galactic B[e] supergiants;Monthly Notices of the Royal Astronomical Society;2018-07-04
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