[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 …

[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 …

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 …

Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae

R Wesson, D Jones, J García-Rojas… - Monthly Notices of …, 2018 - academic.oup.com
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 …

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 …

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 …

Constraints on common envelope magnetic fields from observations of jets in planetary nebulae

J Tocknell, O De Marco, M Wardle - Monthly Notices of the Royal …, 2014 - academic.oup.com
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 …

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 …

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 …

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 …