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A morpho-kinematic and spectroscopic study of the bipolar nebulae: M 2−9, Mz 3, and Hen 2−104

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

Abstract

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.

Citations