The formation of `columns crowns' by jets interacting with a circumstellar dense shell
arXiv:1808.00276 · doi:10.1093/mnras/sty2479
Abstract
We conduct three-dimensional hydrodynamical simulations of two opposite jets that interact with a spherical slow wind that includes a denser shell embedded within it, and obtain a bipolar nebula where each of the two lobes is composed of two connected bubbles and Rayleigh-Taylor instability tongues that protrude from the outer bubble and form the `columns crown'. The jets are launched for a short time of 17 years and inflate a bipolar nebula inside a slow wind. When the bipolar structure encounters the dense shell, the interaction causes each of the two lobes to split to two connected bubbles. The interaction is prone to Rayleigh-Taylor instabilities that form tongues that protrude as columns from the outer bubble. The bases of the columns form a ring on the surface of the outer bubble, and the structure resemble a crown that we term the columns crown. This structure resembles, but is not identical to, the many filaments that protrude from the lobes of the bipolar planetary nebula Menzel~3. We discuss our results in comparison to the structure of Menzel~3 and the ways by which the discrepancies can be reconciled, and possibly turn our failure to reproduce the exact structure of Menzel~3 to a success with jets-shell interaction simulations that include more ingredients.
Accepted to MNRAS
References in corpus (24)
- The impact of companions on stellar evolution
- Accretion in common envelope evolution
- Pre-explosion spiral mass loss of a binary star merger
- Runaway Coalescence at the Onset of Common Envelope Episodes
- Common Envelope Shaping of Planetary Nebulae
- Self-regulating jets during the Common Envelope phase
- The Effect of Tides on the Population of PN from Interacting Binaries
- High-resolution observations of IRAS 08544-4431. Detection of a disk orbiting a post-AGB star and of a slow disk wind
- Shaping Planetary Nebulae by Light Jets
- Binary Central Stars of Planetary Nebulae Discovered Through Photometric Variability V: The Central Stars of HaTr 7 and ESO 330-9
- IFU spectroscopy of southern PNe: III
- SALT HRS discovery of the binary nucleus of the Etched Hourglass Nebula MyCn 18
- The planetary nebula IC 4776 and its post-common-envelope binary central star
- A Model for the Formation of Large Circumbinary Disks Around Post AGB Stars
- Forming H-shaped and barrel-shaped nebulae with interacting jets
- A new look inside Planetary Nebula LoTr 5: A long-period binary with hints of a possible third component
- Observations and 3D Hydrodynamical models of planetary nebulae with Wolf Rayet type central stars
- Models of the Hydrodynamic Histories of post-AGB Stars. I. Multiflow Shaping of OH231.8+04.2
- The binary fraction of planetary nebula central stars: the promise of VPHAS+
- Herschel Planetary Nebula Survey (HerPlaNS): Hydrogen Recombination Laser Lines in Mz 3
- IFU spectroscopy of southern PN VI: The extraordinary chemo-dynamics of Hen 2-111
- Models of the Mass-Ejection Histories of pre Planetary Nebulae. II. The Formation of the Butterfly and its Proboscis in M2-9
- A D'-type symbiotic binary in the planetary nebula SMP LMC 88
- The importance of binarity in the formation and evolution of planetary nebulae
Cited by in corpus (13)
- Bipolar Planetary Nebulae from Outflow Collimation by Common Envelope Evolution
- The structure of jets launched from post-AGB binary systems
- Models of the Mass-Ejection Histories of pre Planetary Nebulae, III. The Shaping of Lobes by post-AGB Winds
- Inclined jets inside a common envelope of a triple stellar system
- Panchromatic HST/WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae. I. NGC 6302
- Jet parameters for a diverse sample of jet-launching post-AGB binaries
- Fast Ejecta Resulted from Jet-Wind Interaction in the Great Eruption of Eta Carinae
- Shaping `Ears' in planetary nebulae by early jets
- Simulating the shaping of point-symmetric structures in the jittering jets explosion mechanism
- Variable jets at the termination of the common envelope evolution
- A companion star launching jets in the wind acceleration zone of a giant star
- On the nature of jets from a main sequence companion at the onset of common envelope evolution
- [Fe II] 1.644m imaging survey of planetary nebulae with low-ionisation structures