2008/02/29 by O. M. Umurhan
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809504
Accepted (July 21, 2008), now in final form
openalex publication_date 2008/07/28 · arxiv created 2008/09/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Context. We present a scaling argument that we develop into a shallow water theory of non-axisymmetric disturbances in annular sections of thin Keplerian disks.