Shock-wave propagation in the nonuniform interstellar medium
1995; American Physical Society; Volume: 67; Issue: 3 Linguagem: Inglês
10.1103/revmodphys.67.661
ISSN1539-0756
AutoresГ. С. Бисноватый-Коган, Sergiy Silich,
Tópico(s)Astrophysics and Star Formation Studies
ResumoThe development of different analytical and approximate numerical methods for calculations of shock-wave propagation in the inhomogeneous interstellar medium is reviewed. The models of ultracompact H II regions, nonspherical supernova remnants, bubbles produced by stellar winds of hot stars, and expanding supershells are discussed on the basis of these calculations.
Referência(s)