[HTML][HTML] Bipolar outflows and the evolution of stars
A Frank - New Astronomy Reviews, 1999 - Elsevier
Hypersonic bipolar outflows are a ubiquitous phenomena associated with both young and
highly evolved stars. Observations of Planetary Nebulae, the nebulae surrounding …
highly evolved stars. Observations of Planetary Nebulae, the nebulae surrounding …
[HTML][HTML] Giant Herbig-Haro Flows
B Reipurth, J Bally, D Devine - Astronomical Journal v. 114, p …, 1997 - adsabs.harvard.edu
Giant Herbig-Haro Flows ADS Classic is now deprecated. It will be completely retired in October
2019. This page will automatically redirect to the new ADS interface at that point. SAO/NASA …
2019. This page will automatically redirect to the new ADS interface at that point. SAO/NASA …
Properties that cannot be explained by the progenitors of planetary nebulae
N Soker - The Astrophysical Journal Supplement Series, 1997 - iopscience.iop.org
ABSTRACT I classify a large number of planetary nebulae (458) according to the process
that caused their progenitors to blow axisymmetrical winds. The classification is based …
that caused their progenitors to blow axisymmetrical winds. The classification is based …
Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae
It has recently been noted that there seems to be a strong correlation between planetary
nebulae with close binary central stars and highly enhanced recombination line …
nebulae with close binary central stars and highly enhanced recombination line …
An interacting binary system powers precessing outflows of an evolved star
HMJ Boffin, B Miszalski, T Rauch, D Jones… - Science, 2012 - science.org
Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when
ejected near the end of their lives. This quirk is most notable during the planetary nebula …
ejected near the end of their lives. This quirk is most notable during the planetary nebula …
Low-ionization structures in planetary nebulae: confronting models with observations
DR Goncalves, RLM Corradi… - The Astrophysical …, 2001 - iopscience.iop.org
Around 50 planetary nebulae (PNs) are presently known to possess" small-scale" low-
ionization structures (LISs) located inside or outside their main nebular bodies. We consider …
ionization structures (LISs) located inside or outside their main nebular bodies. We consider …
Constraints on common envelope magnetic fields from observations of jets in planetary nebulae
The common envelope (CE) interaction describes the swallowing of a nearby companion by
a growing, evolving star. CEs that take place during the asymptotic giant branch phase of the …
a growing, evolving star. CEs that take place during the asymptotic giant branch phase of the …
Photo-evaporation of clumps in planetary nebulae
G Mellema, AC Raga, J Cantó, P Lundqvist… - arXiv preprint astro-ph …, 1997 - arxiv.org
We study the evolution of dense neutral clumps located in the outer parts of planetary
nebulae. These clumps will be photo-ionized by the ionizing radiation from the central star …
nebulae. These clumps will be photo-ionized by the ionizing radiation from the central star …
The MUSE view of the planetary nebula NGC 3132
A Monreal-Ibero, JR Walsh - Astronomy & Astrophysics, 2020 - aanda.org
Aims. Two-dimensional spectroscopic data for the whole extent of the NGC 3132 planetary
nebula have been obtained. We deliver a reduced data-cube and high-quality maps on a …
nebula have been obtained. We deliver a reduced data-cube and high-quality maps on a …
Tomography of the unique ongoing jet in the planetary nebula NGC 2392
MA Guerrero, S Cazzoli, JS Rechy-García… - The Astrophysical …, 2021 - iopscience.iop.org
Jets (fast collimated outflows) are claimed to be the main shaping agent of the most
asymmetric planetary nebulae (PNs), as they impinge on the circumstellar material at late …
asymmetric planetary nebulae (PNs), as they impinge on the circumstellar material at late …