Low-Mass Binary Induced Outflows from Asymptotic Giant Branch Stars

Abstract

A significant fraction of planetary nebulae (PNe) and proto-planetary nebulae (PPNe) exhibit aspherical, axisymmetric structures, many of which are highly collimated. The origin of these structures is not entirely understood, however recent evidence suggests that many observed PNe harbor binary systems, which may play a role in their shaping. In an effort to understand how binaries may produce such asymmetries, we study the effect of low-mass (< 0.3 M_sun) companions (planets, brown dwarfs and low-mass main sequence stars) embedded into the envelope of a 3.0 M_sun star during three epochs of its evolution (Red Giant Branch, Asymptotic Giant Branch (AGB), interpulse AGB). We find that common envelope evolution can lead to three qualitatively different consequences: (i) direct ejection of envelope material resulting in a predominately equatorial outflow, (ii) spin-up of the envelope resulting in the possibility of powering an explosive dynamo driven jet and (iii) tidal shredding of the companion into a disc which facilitates a disc driven jet. We study how these features depend on the secondary's mass and discuss observational consequences.

24 pages, 6 figures, submitted to MNRAS

References in corpus (24)

• Towards Spectral Classification of L and T Dwarfs: Infrared and Optical Spectroscopy and Analysis
• The Spectra of T Dwarfs I: Near-Infrared Data and Spectral Classification
• Double Core Evolution X. Through the Envelope Ejection Phase
• Imaging the circumstellar envelopes of AGB stars
• Dynamos in Asymptotic-Giant-Branch Stars As the Origin of Magnetic Fields Shaping Planetary Nebulale
• A magnetically collimated jet from an evolved star
• On the Binding Energy Parameter of Common Envelope Evolution. Dependency on the Definition of the Stellar Core Boundary during Spiral-in
• MHD Stellar and Disk Winds: Application to Planetary Nebulae
• Properties of the close binary and circumbinary torus of the Red Rectangle
• Indications of a Large Fraction of Spectroscopic Binaries Among Nuclei of Planetary Nebulae
• Why Magnetic Fields Cannot be the Main Agent Shaping Planetary Nebulae
• Discovery of magnetic fields in central stars of planetary nebulae
• The Formation of Cataclysmic Variables with Brown Dwarf Secondaries
• Turbulent Dynamo in Asymptotic Giant Branch Stars
• The Effects of Planets and Brown Dwarfs on Stellar Rotation and Mass-Loss
• Extrasolar Planets and the Rotation and Axisymmetrical mass loss of evolved stars
• High-Resolution Near-Infrared Imaging and Polarimetry of Four Proto-Planetary Nebulae
• A Possible Hidden Population of Spherical Planetary Nebulae
• The Shaping of the Red Rectangle Proto-Planetary Nebula
• The Evidence for a Binary origin of the Young Planetary Nebula HB 12
• Spherical Planetary Nebulae
• Proper Motion and Kinematics of the Ansae in NGC7009
• Extracting Rotational Energy in Supernova Progenitors: Transient Poynting Flux Growth vs. Turbulent Dissipation
• Spitzer detections of new dust components in the outflow of the Red Rectangle

Cited by in corpus (165)

• Pulsational Pair-Instability Supernovae
• A Circumbinary Disk in the Final Stages of Common Envelope and the Core-Degenerate Scenario for Type Ia Supernovae
• Foretellings of Ragnarök: World-engulfing Asymptotic Giants and the Inheritance of White Dwarfs
• Hot Jupiters and Cool Stars
• On the alpha formalism for the common envelope interaction
• The impact of companions on stellar evolution
• On the Orbits of Low-mass Companions to White Dwarfs and the Fates of the Known Exoplanets
• Binary stars as the key to understanding planetary nebulae
• Binary planetary nebulae nuclei towards the Galactic bulge. II. A penchant for bipolarity and low-ionisation structures
• The jet feedback mechanism (jfm) in stars, galaxies and clusters
• Tides and Tidal Engulfment in Post-Main Sequence Binaries: Period Gaps for Planets and Brown Dwarfs Around White Dwarfs
• Isolated vs. Common Envelope Dynamos in Planetary Nebula Progenitors
• Accretion in common envelope evolution
• The Chandra X-ray Survey of Planetary Nebulae (ChanPlaNS): Probing Binarity, Magnetic Fields, and Wind Collisions
• The formation of high-field magnetic white dwarfs from common envelopes
• Mass Transfer and Disc Formation in AGB Binary Systems
• Hydrodynamic Simulations of the Interaction between Giant Stars and Planets
• Magnetic Mixing in Red Giant and Asymptotic Giant Branch Stars
• An Interacting Binary System Powers Precessing Outflows of an Evolved Star
• Jets and Tori in Proto-Planetary Nebulae
• ALMA observations of the nearby AGB star L2 Puppis - I. Mass of the central star and detection of a candidate planet
• Common Envelope Shaping of Planetary Nebulae
• The Red Rectangle: Its Shaping Mechanism and its Source of Ultraviolet Photons
• Magnetic Field Amplification During the Common Envelope Phase
• Single Rotating Stars and the Formation of Bipolar Planetary Nebula
• ETHOS 1: A high latitude planetary nebula with jets forged by a post common envelope binary central star
• Speaking with one voice: simulations and observations discuss the common envelope $\alpha$ parameter
• ALMA imaging of the nascent planetary nebula IRAS 15103-5754
• Three-dimensional hydrodynamical simulations of mass transfer in binary systems by a free wind
• Using Kinematic Properties of Pre-Planetary Nebulae to Constrain Engine Paradigms
• A carbon dwarf wearing a Necklace: first proof of accretion in a post-common-envelope binary central star of a planetary nebula with jets
• The dust disk and companion of the nearby AGB star L2 Puppis - SPHERE/ZIMPOL polarimetric imaging at visible wavelengths
• Discovery of close binary central stars in the planetary nebulae NGC 6326 and NGC 6778
• Planet formation from the ejecta of common envelopes
• The post-common envelope central stars of the planetary nebulae Henize 2-155 and Henize 2-161
• The Effect of Tides on the Population of PN from Interacting Binaries
• Proof of polar ejection fom the close-binary core of the planetary nebula Abell 63
• Connecting planets around horizontal branch stars with known exoplanets
• The Role of Convection in Determining the Ejection Efficiency of Common Envelope Interactions
• Bipolar Planetary Nebulae from Outflow Collimation by Common Envelope Evolution
• Bipolar planetary nebulae from common envelope evolution of binary stars
• Low-ionization structures in planetary nebulae - I: physical, kinematic and excitation properties
• Imaging the circumstellar dust around AGB stars with PolCor
• Minkowski's Footprint revisited. Planetary Nebula formation from a single sudden event?
• The Formation and Evolution of Wind-Capture Disks In Binary Systems
• From Bipolar to Elliptical: Simulating the Morphological Evolution of Planetary Nebulae
• Wide Binary Effects on Asymmetries in Asymptotic Giant Branch Circumstellar Envelopes
• A morpho-kinematic and spectroscopic study of the bipolar nebulae: M 2-9, Mz 3, and Hen 2-104
• The role of planets in shaping planetary nebulae
• Abell 41: shaping of a planetary nebula by a binary central star?
• PPN as Explosions: Bullets vs Jets and Nebular Shaping
• The Formation of Crystalline Dust in AGB Winds from Binary Induced Spiral Shocks
• Wind morphology around cool evolved stars in binaries: the case of slowly accelerating oxygen-rich outflows
• Possible Implications of the Planet Orbiting the Red Horizontal Branch Star HIP 13044
• Spitzer 24 um Survey for Dust Disks around Hot White Dwarfs
• Are Proto-Planetary Nebulae Shaped by a Binary? Results of a Long-Term Radial Velocity Study
• Wind-accelerated orbital evolution in binary systems with giant stars
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• A dense disk of dust around the born-again Sakurai's object
• SPH modelling of companion-perturbed AGB outflows including a new morphology classification scheme
• The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star
• How Drag Force Evolves in Global Common Envelope Simulations
• Two rings but no fellowship: LoTr 1 and its relation to planetary nebulae possessing barium central stars
• ALMA detection of a tentative nearly edge-on rotating disk around the nearby AGB star R~Doradus
• Convection and Spin-Up During Common Envelope Evolution: The Formation of Short-Period Double White Dwarfs
• The planetary nebula IPHASXJ211420.0+434136 (Ou5): insights into common-envelope dynamical and chemical evolution
• NGC 6778: a disrupted planetary nebula around a binary central star
• An evla and carma study of dusty disks and torii with large grains in dying stars
• Evidence of a Binary-Induced Spiral from an Incomplete Ring Pattern of CIT 6
• Modelling the structure and kinematics of the Firework nebula: The nature of the GK Persei nova shell and its jet-like feature
• Gas and Dust Associated with the Strange, Isolated, Star BP Piscium
• Nonlinear Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium
• Hu1-2: a metal-poor bipolar planetary nebula with fast collimated outflows
• Common continuum polarization properties: a possible link between proto-planetary nebulae and Type Ia Supernovae progenitors
• Successive common envelope events from multiple planets
• Convection Reconciles the Difference in Efficiencies Between Low-Mass and High-Mass Common Envelopes
• Three-dimensional hydrodynamic simulations of L2 Puppis
• Forming H-shaped and barrel-shaped nebulae with interacting jets
• Rotating Stars and the Formation of Bipolar Planetary Nebulae II: Tidal Spin-up
• A Substantial Dust Disk Surrounding an Actively Accreting First-Ascent Giant Star
• The Shapes of AGB Envelopes as Probes of Binary Companions
• A study of the kinematics and binary-induced shaping of the planetary nebula HaTr 4
• Spinning-Up the Envelope Before Entering a Common Envelope Phase
• Time-variable non-thermal emission in the planetary nebula IRAS 15103-5754
• Identification of Very Red Counterparts of SiO Maser and OH/IR Objects in the GLIMPSE Survey
• A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b
• Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2
• Accounting for planet-shaped planetary nebulae
• Spatio-kinematic modelling of Abell 65, a double-shelled planetary nebula with a binary central star
• Unusual shock-excited OH maser emission in a young Planetary Nebula
• ALMA observations of the nearby AGB star L${}_2$ Puppis. II. Gas disk properties derived from ${}^{12}$CO and ${}^{13}$CO $J=$3$-$2 emission
• Magnetic Activity in Stellar Merger Products
• The circumstellar envelope around the S-type AGB star W Aql Effects of an eccentric binary orbit
• Inclined jets inside a common envelope of a triple stellar system
• The Exotic Eclipsing Nucleus of the Ring Planetary Nebula SuWt2
• A collimated, ionized bipolar structure and a high density torus in the young planetary nebula IRAS 17347-3139
• HD101584: Circumstellar characteristics and evolutionary status
• Mapping Excitation in the Inner Regions of the Planetary Nebula NGC 5189 using HST WFC3 Imaging
• Common Envelope Shaping of Planetary Nebulae. IV. From Proto-planetary to Planetary Nebula
• Disk evaporation in a planetary nebula
• Kinematics of the ring-like nebula SuWt 2
• Shaping planetary nebulae with jets in inclined triple stellar systems
• Polarization properties of OH emission in planetary nebulae
• Constraining planet formation around 6$M_{\odot }$-8$M_{\odot }$ stars
• Magnetic Nested-wind Scenarios for Bipolar Outflows: Pre-planetary and YSO nebular shaping
• Rapidly-evolving episodic outflow in IRAS 18113-2503: clues to the ejection mechanism of the fastest water fountain
• An outburst powered by the merging of two stars inside the envelope of a giant
• Resolved imaging of the AR Puppis circumbinary disk
• Maser and Infrared Studies of Oxygen-Rich Late/Post-AGB Stars and Water Fountains: Development of a New Identification Method
• Hydrodynamic Simulations of Disrupted Planetary Accretion Discs Inside the Core of an AGB Star
• Binaries traveling through a gaseous medium: Dynamical drag forces and internal torques
• Morpho-kinematic properties of Wolf-Rayet planetary nebulae
• The binary central star of the bipolar pre-planetary nebula IRAS 08005-2356 (V510 Pup)
• Dust formation in common envelope binary interactions -- II: 3D simulations with self-consistent dust formation
• On the role of reduced wind mass-loss rate in enabling exoplanets to shape planetary nebulae
• The Class of Jsolated Stars and Luminous Planetary Nebulae in old stellar populations
• Precessing planetary magnetospheres in SiO stars ? First detection of quasi-periodic polarization fluctuations in R Leo and V Cam
• Revised Stellar Parameters for V471 Tau, A Post-common Envelope Binary in the Hyades
• Planet formation in post-common-envelope binaries
• Dynamical friction in a gaseous medium with a large-scale magnetic field
• Molecules in the Circumstellar Disk Orbiting BP Piscium
• The future influence of six exoplanets on the envelope properties of their parent stars on the giant branches
• Mapping circumstellar magnetic fields of late-type evolved stars with the Goldreich-Kylafis effect: CARMA observations at $\lambda 1.3$ mm of R Crt and R Leo
• The kinematics of the quadrupolar nebula M1-75 and the identification of its central star
• Planetary Nebulae with UVIT II: Revelations from FUV vision of Butterfly Nebula NGC 6302
• VLT observations of the asymmetric Etched Hourglass Nebula, MyCn 18
• The Formation of Discs in the Interior of AGB Stars from the Tidal Disruption of Planets and Brown Dwarfs
• Flickering in AGB stars: Probing the nature of accreting companions
• The enigmatic central star of the planetary nebula PRTM 1
• Variable jets at the termination of the common envelope evolution
• Do Type Ia Supernovae Explode Inside Planetary Nebulae?
• Two-wind interactions in binaries with two orbiting giant stars
• Towards a Spectral Technique for Determining Material Geometry Around Evolved Stars: Application to HD 179821
• Central Stars of Planetary Nebulae
• The Creation of AGB Fallback Shells
• Rapid expansion of red giant stars during core helium flash by waves propagation to the envelope and implications to exoplanets
• Planetary Nebulae: What can they tell us about close binary evolution?
• The Next Generation Virgo Cluster Survey. XVII. A Search for Planetary Nebulae in Virgo Cluster Globular Clusters
• Polarisation of molecular lines in the circumstellar envelope of the post-Asymptotic Giant Branch star OH 17.7-2.0
• Planetary nebulae with Wolf-Rayet-type central stars -- II. Dissecting the compact planetary nebula M2-31 with GTC MEGARA
• Common envelope: progress and transients
• Two circumstellar nebulae discovered with the Wide-field Infrared Survey Explorer and their massive central stars
• The Near-Infrared Polarization of the Pre-Planetary Nebula Frosty Leo
• A Binary Scenario for the Formation of Strongly Magnetized White Dwarfs
• Accretion of Planetary Material onto Host Stars
• Magnetic Fields in Paradigms of Planetary Nebulae and Related MHD Frontiers
• The peculiar molecular envelope around the post-AGB star IRAS 08544--4431
• Stochastic Wobble of Accretion Discs and Jets from Turbulent Rocket Torques
• Second-generation planet formation after tidal disruption from common envelope evolution
• A study of radial self-similar non-relativistic MHD outflow models: parameter space exploration and application to the water fountain W43A
• Infrared interferometric imaging of the compact dust disk around the AGB star HR3126 with the bipolar Toby Jug Nebula
• Extreme Climate Variations from Milankovitch-like Eccentricity Oscillations in Extrasolar Planetary Systems
• Jet Power in Pre-Planetary Nebulae: Observations vs. Theory
• Mass transfer in asymptotic-giant-branch binary systems
• Observations of dusty torii and compact disks around evolved stars: the high spatial resolution IR view
• Light Curve Models of Convective Common Envelopes
• Post-AGB nebular studies
• Two Populations of Companions around White Dwarfs: The Effect of Tides and Tidal Engulfment
• Olivier Chesneau's work on low mass stars
• Kinematical Properties of Planetary Nebulae with WR-type Nuclei
• Size of discs formed by wind accretion in binaries can be underestimated if the role of wind-driving force is ignored
• Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
• The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses
• 3D models of the circumstellar environments of evolved stars: Formation of multiple spiral structures
• Morphologies of Wolf-Rayet Planetary Nebulae based on IFU Observations