Observational Effects of Anomalous Boundary Layers in Relativistic Jets
arXiv:0803.2693 · doi:10.1086/588605
Abstract
Recent theoretical work has pointed out that the transition layer between a jet an the medium surrounding it may be more complex than previously thought. Under physically realizable conditions, the transverse profile of the Lorentz factor in the boundary layer can be non-monotonic, displaying the absolute maximum where the flow is faster than at the jet spine, followed by an steep fall off. Likewise, the rest-mass density, reaches an absolute minimum (coincident with the maximum in Lorentz factor) and then grows until it reaches the external medium value. Such a behavior is in contrast to the standard monotonic decline of the Lorentz factor (from a maximum value at the jet central spine) and the corresponding increase of the rest-mass density (from the minimum reached at the jet core). We study the emission properties of the aforementioned anomalous shear layer structures in kiloparsec-scale jets aiming to show observable differences with respect to conventional monotonic and smooth boundary layers.
arXiv comment32 pages, 9 figures (1 in color), accepted in ApJ
References in corpus (40)
- Relativistic Jets from Collapsars
- Relativistic outflows from remnants of compact object mergers and their viability for short gamma-ray bursts
- X-ray Emission Properties of Large Scale Jets, Hotspots and Lobes in Active Galactic Nuclei
- GENESIS: A high-resolution code for 3D relativistic hydrodynamics
- Optical and Radio Polarimetry of the M87 Jet at 0.2" Resolution
- Chandra X-ray Observations of Pictor A: High Energy Cosmic Rays in a Radio Galaxy?
- Radiation from the Relativistic Jet: a Role of the Shear Boundary Layer
- Chandra observations of the X-ray jet in 3C66B
- Disk-Jet Coupling in Black Hole Accretion Systems I: General Relativistic Magnetohydrodynamical Models
- Shear acceleration in relativistic astrophysical jets
- Chandra finds X-ray jets are common in low-power radio galaxies
- Radio Jet-Ambient Medium Interactions on Parsec Scales in the Blazar 1055+018
- Neutrino pair annihilation near accreting, stellar-mass black holes
- Chandra Discovery of a 300 kpc X-ray Jet in the GPS Quasar PKS1127-145
- 3D Simulations of Relativistic Precessing Jets Probing the Structure of Superluminal Sources
- High--Resolution 3D Simulations of Relativistic Jets
- New results on particle acceleration in the Centaurus A jet and counterjet from a deep Chandra observation
- Stability Properties of Strongly Magnetized Spine Sheath Relativistic Jets
- Collimation of astrophysical jets - the role of the accretion disk magnetic field distribution
- A powerful hydrodynamic booster for relativistic jets
- Radio Emission from 3D Relativistic Hydrodynamic Jets: Observational Evidence of Jet Stratification
- Controlling the collimation and rotation of hydromagnetic disk winds
- The Chandra view of extended X-ray emission from Pictor A
- Chandra discovery of extended non-thermal emission in 3C 207 and the spectrum of the relativistic electrons
- On possible `cosmic ray cocoons' of relativistic jets
- The X-ray Jet in Centaurus A: Clues on the Jet Structure and Particle Acceleration
- Resonant Kelvin-Helmholtz modes in sheared relativistic flows
- On the Magnetic Field in the Kiloparsec-Scale Jet of Radio Galaxy M 87
- Ultra-Relativistic Magneto-Hydro-Dynamic Jets in the context of Gamma Ray Bursts
- Synthetic X-ray light curves of BL Lacs from relativistic hydrodynamic simulations
- Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts
- Transverse stability of relativistic two-component jets
- Internal shocks in relativistic outflows: collisions of magnetized shells
- The exact solution of the Riemann problem in relativistic MHD with tangential magnetic fields
- Which physical parameters can be inferred from the emission variability of relativistic jets?
- Is the High-Energy Emission from Centaurus A Compton-Scattered Jet Radiation?
- The jets in 3C 296
- The structure of the jet in 3C 15 from multi-band polarimetry
- An Efficient Implementation of Flux Formulae in Multidimensional Relativistic Hydrodynamical Codes
- Generation of the magnetic field in jets
Cited by in corpus (24)
- The Jets of TeV Blazars at Higher Resolution: 43 GHz and Polarimetric VLBA Observations from 2005-2009
- Synchrotron radiation of self-collimating relativistic MHD jets
- Three-Dimensional Relativistic Magnetohydrodynamic Simulations of Current-Driven Instability. III. Rotating Relativistic Jets
- Stability of three-dimensional relativistic jets: implications for jet collimation
- An Introduction to Particle Acceleration in Shearing Flows
- Ultrahigh-energy Cosmic-ray Nuclei from Black Hole Jets: Recycling Galactic Cosmic Rays through Shear Acceleration
- Magnetohydrodynamic Effects in Propagating Relativistic Jets: Reverse Shock and Magnetic Acceleration
- On the dynamic efficiency of internal shocks in magnetized relativistic outflows
- Cen A as TeV gamma-ray and possible UHE cosmic-ray source
- Chandra Reveals Twin X-ray Jets in the Powerful FR-II Radio Galaxy 3C353
- Multiwavelength afterglow light curves from magnetized GRB flows
- Striped Blandford/Znajek jets from advection of small scale magnetic field
- Radiative signature of magnetic fields in internal shocks
- Linear Theory of the Rayleigh-Taylor Instability at a Discontinuous Surface of a Relativistic Flow
- Shocks in relativistic transverse stratified jets, a new paradigm for radio-loud AGN
- VLBI-selected sample of Compact Symmetric Object candidates and frequency-dependent position of hotspots
- The magnetohydrodynamic instability of current-carrying jets
- Effect of Interacting Rarefaction Waves on Relativistically Hot Jets
- Shear Acceleration in Expanding Flows
- Novel Analysis of the Multiwavelength Structure of Relativistic Jet in Quasar 3C 273
- The influence of the magnetic field on the spectral properties of blazars
- Scaling of the Anomalous Boost in Relativistic Jet Boundary Layer
- On the influence of a Hybrid Thermal-Non thermal distribution in the Internal Shocks model for blazars
- Magnetization of Relativistic Current-Carrying Jets with Radial Velocity Shear