Emission profile variability in hot star winds. A pseudo 3D method based on radiation hydrodynamics simulations

L. Dessart, S.P. Owocki

Research output: Contribution to journalArticleAcademicpeer-review

Original languageUndefined/Unknown
Pages (from-to)1113
Number of pages1
JournalAstronomy and Astrophysics
Volume383
Publication statusPublished - 2002

Cite this