Space Velocity and Time Span of Jets in Planetary Nebulae
Martin A Guerrero, Jackeline S Rechy-Garcia, Roberto Ortiz

TL;DR
This study statistically analyzes jets in planetary nebulae, revealing two main velocity populations, their interaction with nebular envelopes, and their typical lifespan of less than 2,500 years, showing jets are generally coeval with their nebulae.
Contribution
It provides the first orientation-independent statistical analysis of jet velocities, ages, and interactions in planetary nebulae, revealing two distinct velocity groups and their evolutionary implications.
Findings
70% of jets have velocities below 100 km/s
Most jets are coeval with their planetary nebulae (1,000-3,000 yrs old)
Jets have a typical lifespan shorter than 2,500 years
Abstract
Fast highly-collimated outflows including bipolar knots, jet-like features, and point-symmetric filaments or string of knots are common in planetary nebulae (PNe). These features, generally named as jets, are thought to play an active role in the nebular shaping immediately before or at the same time that fast stellar winds and D-type ionization fronts shock and sweep up the nebular envelope. The space velocity, radial distance from the central star and kinematic age of jets in PNe cannot be determined because the inclination anglewith the line-of-sight is usually unknown. Here we have used the large number of jets already detected in PNe to derive orientation-independent properties from a statistical point of view. We find that jets in PNe can be assigned to two different populations: a significant fraction (70%) have space velocities below 100 km s, whereas only…
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