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G.Brunetti

Identifiers

  • name variant G.Brunetti 0.60 · backfill

Papers (15)

  1. The nature of the low-frequency emission of M51: First observations of a nearby galaxy with LOFAR astro-ph.GA · 2014 · author #11
  2. A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures astro-ph.CO · 2011 · author #4
  3. Massive and Refined. II. The statistical properties of turbulent motions in massive galaxy clusters with high spatial resolution astro-ph.CO · 2010 · author #2
  4. High energy emission from galaxy clusters and particle acceleration due to MHD turbulence astro-ph.HE · 2009 · author #1
  5. Shock Waves in Eulerian Cosmological Simulations: Main Properties and Acceleration of Cosmic Rays astro-ph · 2008 · author #2
  6. Cosmological Shocks in Eulerian Simulations: Main Properties and Cosmic Rays Acceleration astro-ph · 2008 · author #2
  7. Radio Lobes of Pictor A: an X-ray spatially resolved Study astro-ph · 2007 · author #4
  8. The cluster relic source in A521 astro-ph · 2005 · author #4
  9. Chandra detects inverse Compton emission from the radio galaxy 3C 219 astro-ph · 2002 · author #1
  10. Chandra discovery of extended non-thermal emission in 3C 207 and the spectrum of the relativistic electrons astro-ph · 2001 · author #1
  11. Chandra detection of the radio and optical double hot spot of 3C 351 astro-ph · 2001 · author #1
  12. Hard X-ray emission from the galaxy cluster A3667 astro-ph · 2001 · author #4
  13. Anisotropic inverse Compton scattering in powerful radio galaxies: the case of 3C 295 astro-ph · 2001 · author #1
  14. Particle injection and reacceleration in clusters of galaxies and the EUV excess: the case of Coma astro-ph · 2000 · author #1
  15. Anisotropic inverse Compton scattering in radio galaxies and particle energy distribution astro-ph · 2000 · author #1

Mentions

  • 0901.1432 #1 · backfill · confidence 0.70 G.Brunetti
  • 0808.0609 #2 · backfill · confidence 0.70 G.Brunetti
  • 0805.4214 #2 · backfill · confidence 0.70 G.Brunetti
  • 0704.2131 #4 · backfill · confidence 0.70 G.Brunetti

Frequent Coauthors