Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Fermi Detection Of The Pulsar Wind Nebula Hess J1640–465

Journal Article · · The Astrophysical Journal
 [1];  [2];  [3];  [3];  [4];  [5];  [6]
  1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Univ. Simon Bolivar (Venezuela)
  3. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  4. Inst. de Physique Nucleaire (IPN), Orsay (France)
  5. New York Univ. (NYU), NY (United States)
  6. Univ. of Bordeaux, Gradignan (France)

We present observations of HESS J1640–465 with the Fermi-Large Area Telescope. The source is detected with high confidence as an emitter of high-energy gamma-rays. The spectrum lacks any evidence for the characteristic cutoff associated with emission from pulsars, indicating that the emission arises primarily from the pulsar wind nebula (PWN). Broadband modeling implies an evolved nebula with a low magnetic field resulting in a high γ-ray to X-ray flux ratio. The Fermi emission exceeds predictions of the broadband model, and has a steeper spectrum, possibly resulting from a distinct excess of low energy electrons similar to what is inferred for both the Vela X and Crab PWNe.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1357537
Alternate ID(s):
OSTI ID: 21460139
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 720; ISSN 0004-637X
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

References (32)

Was SN 1054 a Type II Supernova? book January 1977
Nuclear enhancement factor in calculation of Galactic diffuse gamma-rays: A new estimate with DPMJET-3 journal June 2009
Multiband emission from pulsar wind nebulae: a possible injection spectrum journal June 2010
Re-examining the X-ray versus spin-down luminosity correlation of rotation powered pulsars journal May 2002
GMRT radio observations of HESS J1640-465
  • Giacani, E.; Castelletti, G.; Dubner, G.
  • HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy, AIP Conference Proceedings https://doi.org/10.1063/1.3076648
conference January 2008
Evolution of pulsar-driven supernova remnants journal March 1984
The expected high-energy to ultra-high-energy gamma-ray spectrum of the Crab Nebula journal September 1992
The Likelihood Analysis of EGRET Data journal April 1996
Diffuse Continuum Gamma Rays from the Galaxy journal July 2000
Nonthermal Emission from a Supernova Remnant in a Molecular Cloud journal July 2000
Evolution of Nonradiative Supernova Remnants journal February 1999
The Third EGRET Catalog of High‐Energy Gamma‐Ray Sources journal July 1999
The H.E.S.S. Survey of the Inner Galaxy in Very High Energy Gamma Rays journal January 2006
Parameterization of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\gamma ,\, e^{\pm }$ \end{document} , and Neutrino Spectra Produced by p‐p Interaction in Astronomical Environments journal August 2006
XMM‐Newton Observations Reveal the X‐Ray Counterpart of the Very High Energy Gamma‐Ray Source HESS J1640−465 journal June 2007
The Infrared Detection of the Pulsar Wind Nebula in the Galactic Supernova Remnant 3C 58 journal March 2008
Particle Acceleration in Relativistic Collisionless Shocks: Fermi Process at Last? journal July 2008
Probing the Nature of the Vela X Cocoon journal November 2008
Probing the Radio to X-Ray Connection of the Vela X Pulsar Wind Nebula with Fermi LAT and H.E.S.S. journal November 2008
THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION journal May 2009
A Dynamical Model for the Evolution of a Pulsar wind Nebula Inside a Nonradiative Supernova Remnant journal September 2009
FERMI LAT DISCOVERY OF EXTENDED GAMMA-RAY EMISSION IN THE DIRECTION OF SUPERNOVA REMNANT W51C journal October 2009
High-Resolution X-Ray Observations of the Pulsar wind Nebula Associated with the Gamma-Ray Source hess J1640–465 journal November 2009
FERMI LARGE AREA TELESCOPE DETECTION OF PULSED γ-RAYS FROM THE VELA-LIKE PULSARS PSR J1048–5832 AND PSR J2229+6114 journal November 2009
Nonthermal Radiation of Young Supernova Remnants: the case of rx J1713.7–3946 journal December 2009
Efficient Cosmic ray Acceleration, Hydrodynamics, and Self-Consistent Thermal X-Ray Emission Applied to Supernova Remnant rx J1713.7-3946 journal February 2010
FERMI LARGE AREA TELESCOPE OBSERVATIONS OF THE VELA-X PULSAR WIND NEBULA journal March 2010
FERMI LARGE AREA TELESCOPE OBSERVATIONS OF SUPERNOVA REMNANTS INTERACTING WITH MOLECULAR CLOUDS journal June 2010
FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOG journal May 2010
Gamma-ray emission from SNR RX J1713.7−3946 and the origin of galactic cosmic rays journal January 2009
Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE journal December 2009
The Evolution and Structure of Pulsar Wind Nebulae journal September 2006

Cited By (10)

CHASING THE IDENTIFICATION OF ASCA GALACTIC OBJECTS (ChIcAGO): AN X-RAY SURVEY OF UNIDENTIFIED SOURCES IN THE GALACTIC PLANE. I. SOURCE SAMPLE AND INITIAL RESULTS journal April 2014
HESS J1640-465 - an exceptionally luminous TeV  -ray supernova remnant journal February 2014
Interstellar gas towards the TeV γ-ray sources HESS J1640−465 and HESS J1641−463 journal October 2016
Non-thermal emission from pulsar-wind nebulae in starburst galaxies journal November 2012
HESS J1640-465 - an exceptionally luminous TeV ${\gamma}$-ray supernova remnant text January 2014
Interstellar gas towards the TeV γ-ray sources HESS J1640−465 and HESS J1641−463 text January 2017
The Dipole Magnetic Field and Spin-down Evolutions of the High Braking Index Pulsar PSR J1640–4631 journal October 2017
Effects of Synchrotron Cooling and Pair Production on Collisionless Relativistic Reconnection journal May 2019
Non-thermal emission from Pulsar-Wind Nebulae in Starburst Galaxies text January 2012
HESS J1640-465 - an exceptionally luminous TeV gamma-ray supernova remnant text January 2014

Similar Records

FERMI DETECTION OF THE PULSAR WIND NEBULA HESS J1640-465
Journal Article · Wed Sep 01 00:00:00 EDT 2010 · Astrophysical Journal · OSTI ID:21460139

NuSTAR discovery of a young, energetic pulsar associated with the luminous gamma-ray source HESS J1640–465
Journal Article · Fri Jun 20 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:22356583

HIGH-RESOLUTION X-RAY OBSERVATIONS OF THE PULSAR WIND NEBULA ASSOCIATED WITH THE GAMMA-RAY SOURCE HESS J1640-465
Journal Article · Mon Nov 30 23:00:00 EST 2009 · Astrophysical Journal · OSTI ID:21378088