Titlebook: Instability and Variability of Hot-Star Winds; Proceedings of an In Anthony F. J. Moffat,Stanley P. Owocki,Nicole St-L Conference proceedin

Deleterious

書目名稱Instability and Variability of Hot-Star Winds影響因子(影響力)




書目名稱Instability and Variability of Hot-Star Winds影響因子(影響力)學(xué)科排名




書目名稱Instability and Variability of Hot-Star Winds網(wǎng)絡(luò)公開(kāi)度




書目名稱Instability and Variability of Hot-Star Winds網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書目名稱Instability and Variability of Hot-Star Winds被引頻次




書目名稱Instability and Variability of Hot-Star Winds被引頻次學(xué)科排名




書目名稱Instability and Variability of Hot-Star Winds年度引用




書目名稱Instability and Variability of Hot-Star Winds年度引用學(xué)科排名




書目名稱Instability and Variability of Hot-Star Winds讀者反饋




書目名稱Instability and Variability of Hot-Star Winds讀者反饋學(xué)科排名

GRUEL

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

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

減至最低

燈泡

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!

交響樂(lè)

mechanism

多山

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

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.