Disk-Driven Planetary Nebulae: Shapes and Spectra
Proceedings of the International Astronomical Union, vol. 19, pp. 422–424
Abstract
Abstract I have performed numerical hydrodynamical calculations of outflows driven by the evaporation of a pseudo-barotropic ring around a luminous central star. The outflow shapes and internal structures resemble known cylindrical nebulae. Some of the corresponding synthetic spectra show ‘Hubble’ type outflow.
Authors 1
-
Affiliation as printed
Universiteit Leiden
Cited by 0 stored of 0
No patents citing this paper on Lens.org (checked 2026-10-11).