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- W837130210 abstract "During the first year of this project, the PI began work in several areas that are expected to yield a substantial increase in our understanding of how and why stars form winds and disks. The approach outlined in the original proposal comprised four complementary pieces (cool and hot stars; observations and theory for each), and the accomplishments in this report are thus divided into these four categories." @default.
- W837130210 created "2016-06-24" @default.
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- W837130210 date "2005-01-01" @default.
- W837130210 modified "2023-09-27" @default.
- W837130210 title "Waves and Turbulence in Stellar Winds across the H-R Diagram" @default.
- W837130210 hasPublicationYear "2005" @default.
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