A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions

Author

Jaylene R. Naylor, The University of MontanaFollow

Year of Award

1999

Document Type

Thesis

Degree Type

Master of Science (MS)

Department or School/College

Department of Physics and Astronomy

Committee Chair

David B. Friend

Keywords

Stellar winds., Mass loss (Astrophysics), Stars Radiation.

Recommended Citation

Naylor, Jaylene R., "A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions" (1999). Graduate Student Theses, Dissertations, & Professional Papers. 8328.
https://scholarworks.umt.edu/etd/8328