A Modified Synchrotron Model for Knots in the M87 Jet
arXiv:0708.3422 · doi:10.1086/522601
Abstract
For explaining the broadband spectral shape of knots in the M87 jet from radio through optical to X-ray, we propose a modified synchrotron model that considers the integrated effect of particle injection from different acceleration sources in the thin acceleration region. This results in two break frequencies at two sides of which the spectral index of knots in the M87 jet changes. We discuss the possible implications of these results for the physical properties in the M87 jet. The observed flux of the knots in the M87 jet from radio to X-ray can be satisfactorily explained by the model, and the predicted spectra from ultraviolet to X-ray could be further tested by future observations. The model implies that the knots D, E, F, A, B, and C1 are unlikely to be the candidate for the TeV emission recently detected in M87.
12 pages, 1 figure, 2 tables, Accepted for publication in ApJ Letters
References in corpus (21)
- The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
- Fast variability of TeV gamma-rays from the radio galaxy M 87
- X-ray Emission from Extragalactic Jets
- A High Resolution X-ray Image of the Jet in M 87
- Chandra X-ray Imaging and Spectroscopy of the M87 Jet and Nucleus
- Optical and Radio Polarimetry of the M87 Jet at 0.2" Resolution
- Is the Giant Radio Galaxy M87 a TeV Gamma-Ray Emitter?
- Dynamics and High Energy Emission of the Flaring HST-1 Knot in the M 87 Jet
- Superluminal Radio Features in the M87 Jet and the Site of Flaring TeV Gamma-ray Emission
- The Outburst of HST-1 in the M87 Jet
- The Optical-Near-IR Spectrum of the M87 Jet From HST Observations
- The X-ray Emissions from the M87 Jet: Diagnostics and Physical Interpretation
- Flaring X-ray Emission from HST-1, a Knot in the M87 Jet
- Intrinsic Curvature in the X-ray Spectra of BL Lacertae Objects
- Month-Timescale Optical Variability in the M87 Jet
- The radio-ultraviolet spectral energy distribution of the jet in 3C273
- Is the core of M87 the source of its TeV emission? Implications for unified schemes
- The Extragalactic Distance Scale Key Project XVIII. The Discovery of Cepheids and a New Distance to NGC 4535 Using the Hubble Space Telescope
- Shock Acceleration of Cosmic Rays - a critical review
- Are Cen a and M87 Tev Gamma-Ray Sources?
- Ultraviolet HST Observations of the Jet in M87
Cited by in corpus (13)
- A Magnetohydrodynamic Model of the M87 Jet I: Superluminal Knot Ejections from HST-1 as Trails of Quad Relativistic MHD Shocks
- Determination of the intrinsic velocity field in the M87 jet
- High Energy Emission Processes in OJ 287 during 2009 Flare
- X-ray Radiation Mechanisms and Beaming Effect of Hot Spots and Knots in Active Galactic Nuclear Jets
- The energy distribution of relativistic electrons in the kilo-parsec scale jet of M87 with Chandra
- A Multiwavelength Spectral and Polarimetric Study of the Jet of 3C 264
- Radio-Gamma-ray connection and spectral evolution in 4C +49.22 (S4 1150+49): the Fermi, Swift and Planck view
- A Two Zone Synchrotron Model for the Knots in the M87 Jet
- A Magnetohydrodynamic Model of The M87 Jet. II. Self-consistent Quad-shock Jet Model for Optical Relativistic Motions and Particle Acceleration
- Examining High Energy Radiation Mechanisms of Knots and Hotspots in Active Galactic Nucleus Jets
- An asymmetrical synchrotron model for knots in the 3C 273 jet
- An hourglass model for the flare of HST-1 in M87
- A Modified Stratified Model for 3C 273 Jet