Shapes and Shaping of Planetary Nebulae
By B. Balick, A. Frank. 2002
518 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/f6239ef0b4df996347241ad3d8753fc8874d808e
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In Astronomy and Astrophysics
- C. Badenes
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Citations in the corpus
- EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF AGB STARS AT DIFFERENT METALLICITIES. III. INTERMEDIATE-MASS MODELS, REVISED LOW-MASS MODELS, AND THE pH-FRUITY INTERFACE (2015, unknown): “Other useful constraints to theoretical models come from the s udy of the abundances derived in Planetary Nebulae (PNe), which lie between the tip of the AGBand the WDs cooling sequence (for a review see Balick & Frank 2002).”
- Magnetic tower outflows from a radial wire array Z-pinch (2005, background): “…occurring in environments as diverse as newly forming stars (Young Stellar Objects: YSOs, Reipurth & Bally 2001), dying solar type stars (Planetary Nebulae, PN Balick & Frank 2002) and supermassive black holes at the center of Active Galactic Nuclei (AGN, see Begelman, Blandford, Rees 1984).”
- Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants? (2007, background): “Continuous bipolar outflows may lead to a bipolar CSM structure similar to some planetary nebulae (Balick & Frank 2002), but this does not seem likely for the objects in our sample.”
- Binary planetary nebulae nuclei towards the Galactic bulge - I. Sample discovery, period distribution, and binary fraction (2009, background): “Binarity offers a simpler or even preferred mechanism to explain non-spherical nebular morphologies such as bipolar PNe (e.g. Soker 1998), but without a firm estimate of the binary fraction other mechanisms cannot be ruled out (for a review of these other mechanisms see Balick & Frank 2002).”
- Keplerian discs around post-AGB stars: a common phenomenon? (2006, background): “…are driving the morphology changes gained even more impetus from the finding that also resolved cooler post-AGB stars or Proto-Planetary Nebulae (PPNe) display a surprisingly wide variety in shapes and structures, very early in their postAGB evolution (Balick & Frank 2002, and references therein).”