output
19922026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations

Showing 2009 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2009★ 72 cited

Localising the VHE gamma-ray source at the Galactic Centre

The HESS Collaboration, F. Acero

The inner 10 pc of our galaxy contains many counterpart candidates of the very high energy (VHE; > 100 GeV) gamma-ray point source HESS J1745-290. Within the point spread function…

astro-ph.GA2009★ 30 cited

The WMAP haze from the Galactic Center region due to massive star explosions and a reduced cosmic ray scale height

Peter L. Biermann, Julia K. Becker, Gabriel Caceres +3

One important prediction of acceleration of particles in the supernova caused shock in the magnetic wind of exploding Wolf Rayet and Red Super Giant stars is the production of an e…

astro-ph.GA2009★ 31 cited

Cosmic-ray driven dynamo in the interstellar medium of irregular galaxies

H. Siejkowski, M. Soida, K. Otmianowska-Mazur +2

Irregular galaxies are usually smaller and less massive than their spiral, S0, and elliptical counterparts. Radio observations indicate that a magnetic field is present in irregula…

astro-ph.GA2009★ 132 cited

Spectrum and variability of the Galactic Center VHE gamma-ray source HESS J1745-290

H. E. S. S. collaboration, :, F. Aharonian

A detailed study of the spectrum and variability of the source HESS J1745-290 in the Galactic Center (GC) region using new data from the H.E.S.S. array of Cherenkov telescopes is p…

astro-ph.GA2009★ 39 cited

PIC simulations of the Thermal Anisotropy-Driven Weibel Instability: Field growth and phase space evolution upon saturation

A Stockem, M E Dieckmann, R Schlickeiser

The Weibel instability is investigated with PIC simulations of an initially unmagnetized and spatially uniform electron plasma. This instability, which is driven by the thermally a…

astro-ph.GA2009★ 37 cited

Local Turbulence Simulations for the Multiphase ISM

R. Kissmann, J. Kleimann, H. Fichtner +1

In this paper we show results of numerical simulations for the turbulence in the interstellar medium. These results were obtained using a Riemann solver-free numerical scheme for h…