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On the hydrogen neutral outflowing disks of B[e] supergiants
M. Kraus
*
, M. Borges Fernandes, F. X. De Araújo
*
Corresponding author for this work
Clinic of Surgery
Federal University of Rio de Janeiro
34
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Keyphrases
B-type
25%
Density Contrast
25%
Dust Emission
25%
Dust Formation
50%
Equatorial Winds
25%
Excess Emissions
25%
Free-free
100%
Good Fit
25%
Infrared Excess
25%
Mass Loss Rate
50%
Minimum Value
25%
Near-infrared Range
25%
Opacity
25%
Optical Emission
25%
Polar Line
25%
Polar Model
25%
Polar Wind
75%
Spectral Energy Distribution
50%
Stellar Surfaces
50%
Wind Model
25%
Physics
Condensation
25%
High Resolution
25%
Infrared Excess
25%
Light Emission
25%
Near Infrared
75%
Spectral Energy Distribution
50%
Stellar Surfaces
50%
Supergiant
100%
INIS
energy distribution
28%
mass loss
28%
opacity
14%
wind
100%