Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic On-line Article (HTML)
· arXiv e-print (arXiv:1210.5841)
· Table of Contents
· References in the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
First LOFAR observations of gamma-ray binaries
Authors:
Marcote, B.; Ribó, M.; Paredes, J. M.; Swinbank, J.; Broderick, J.; Fender, R.; Markoff, S.; Wijers, R.
Affiliation:
AA(Departament d'Astronomia i Meteorologia, Institut de Ciències del Cosmos (ICC), Universitat de Barcelona (IEEC-UB), Spain), AB(Departament d'Astronomia i Meteorologia, Institut de Ciències del Cosmos (ICC), Universitat de Barcelona (IEEC-UB), Spain), AC(Departament d'Astronomia i Meteorologia, Institut de Ciències del Cosmos (ICC), Universitat de Barcelona (IEEC-UB), Spain), AD(Astronomical Institute Anton Pannekoek, University of Amsterdam, Netherlands), AE(School of Physics and Astronomy, University of Southampton, United Kingdom), AF(School of Physics and Astronomy, University of Southampton, United Kingdom), AG(Astronomical Institute Anton Pannekoek, University of Amsterdam, Netherlands), AH(Astronomical Institute Anton Pannekoek, University of Amsterdam, Netherlands)
Publication:
HIGH ENERGY GAMMA-RAY ASTRONOMY: 5th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Volume 1505, pp. 374-377 (2012). (AIPC Homepage)
Publication Date:
12/2012
Origin:
AIP
Abstract Copyright:
(c) 2012: American Institute of Physics
DOI:
10.1063/1.4772275
Bibliographic Code:
2012AIPC.1505..374M

Abstract

A few binary systems display High Energy (100 MeV-100 GeV) and/or Very High Energy (>~ 100 GeV) gamma-ray emission. These systems also display non-thermal radio emission+that can be resolved with long-baseline radio interferometers, revealing the presence of outflows. It is expected that at very low frequencies the synchrotron radio emission covers larger angular scales than has been reported up to now. Here we present preliminary results of the first deep radio observations of the gamma-ray binary LS I +61 303 with LOFAR, which is sensitive to extended structures on arcsecond to arcminute scales.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
  New!

Find Similar Abstracts:

Use: Authors
Title
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints