Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
Year: 1993
Type: article
Source: The Astrophysical Journal
DOI: 10.1086/172676
Authors: J. E. Bjorkman, J. P. Cassinelli
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: closed
OpenAlex ID: W1967847439
