Seismic diagnostics for rotating massive main sequence stars
Abstract
Effects of stellar rotation on adiabatic oscillation frequencies of β Cephei star are discussed. Methods to evaluate them are briefly described and some of the main results for four specific stars are presented.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.