SIMBAD references

2003A&A...399.1121B - Astronomy and Astrophysics, volume 399, 1121-1134 (2003/3-1)

Gamma-ray emission from Wolf-Rayet binaries.

BENAGLIA P. and ROMERO G.E.

Abstract (from CDS):

In the colliding wind region of early-type binaries, electrons can be accelerated up to relativistic energies displaying power-law spectra, as demonstrated by the detection of non-thermal radio emission from several WR+OB systems. The particle acceleration region, located between the stars, is exposed to strong photon fields in such a way that inverse Compton cooling of the electrons could result in a substantial high-energy non-thermal flux. In particular cases, the ratio of the energy densities of magnetic to photon fields in the colliding wind region will determine whether a given source can produce or not significant gamma-ray emission. We present here a study of the binaries WR 140, WR 146, and WR 147 in the light of recent radio and gamma-ray observations. We show that with reasonable assumptions for the magnetic field strength WR 140 can produce the gamma-ray flux from the EGRET source 3EG J2022+4317. WR 146 and WR 147 are below the detection threshold, but new and forthcoming instruments like INTEGRAL and GLAST might detect non-thermal emission from them.

Abstract Copyright:

Journal keyword(s): stars: early-type - stars: binaries: general - stars: winds, outflows - radio continuum: stars - gamma-rays: observations - gamma-rays: theory

Simbad objects: 17

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2003A&A...399.1121B and select 'bookmark this link' or equivalent in the popup menu


2020.01.19-08:25:11

© Université de Strasbourg/CNRS

    • Contact