Deleterious
发表于 2025-3-21 17:32:53
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GRUEL
发表于 2025-3-21 23:54:32
Theory Review: Line-Driven Instability and Other Causes of Structure and Variability in Hot-Star Winively small-scale, stochastic variability, I review the role of the strong intrinsic instability of the line-driving process itself. For larger scale structure, I describe recent efforts to examine how disturbances from the underlying, rotating star can be translated outward into propagating features in the wind.
Aesthete
发表于 2025-3-22 02:19:32
Winds of Magnetic B Starsis known. Magnetic winds are interesting in their own right. In addition, they provide an opportunity to look for unique signatures that can be used to identify magnetic winds in stars where the fields are too weak or complex to be observed directly.
Mystic
发表于 2025-3-22 04:37:59
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减至最低
发表于 2025-3-22 10:41:51
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灯泡
发表于 2025-3-22 16:07:13
e Telescope Science Institute in October, 1991. At that meeting, the four of us collectively decided that the time was ripe for an even more focussed discussion of the basic issues in the area of hot-star wind instability and its observable manifestations. Not that the big problems have been solved!
交响乐
发表于 2025-3-22 18:35:20
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mechanism
发表于 2025-3-22 21:12:25
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多山
发表于 2025-3-23 02:44:55
Observations of Structure in the Stellar Wind of HD 152408 day. Sympathetic variations are apparent in the Balmer emission lines. The observations provide constraints on the stability of the low—velocity stellar wind regime, and indicate the presence of large—amplitude perturbations at great depths in the outflow.
LURE
发表于 2025-3-23 05:42:53
Wind Variability in Intermediate Luminosity B Supergiantsuss a time series for the B0.5 Ib HD 64760 which suggests the long sought after connection between wind and photospheric activity. Newly developed analysis techniques needed to extract physical information from the wind lines are discussed, and results are applied to the time series.