2015/08/05 by N. Clyne, Niall Clyne, Stavros Akras +9
Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Geology #Morpho #Nebula #Optics #Paleontology #Physics #Planetary nebula #Stars #Stellar, planetary, and galactic studies #White dwarf #astro-ph.GA #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201526585
published as A&A 582, A60 (2015) · 15 pages, 7 tables, 9 figures. Accepted for publication by A&A
openalex publication_date 2015/08/05 · arxiv created 2015/09/17 · arxiv updated 2015/10/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context. Complex bipolar shapes can be generated either as a planetary nebula or a symbiotic system. The origin of the material ionised by the white dwarf is very different in these two scenarios, and it complicates the understanding of the morphologies of planetary nebulae.