A possible link between the galactic center hess source and sagittarius a*

D. R. Ballantyne, Fulvio Melia, Siming Liu, Roland M. Crocker

Research output: Contribution to journalArticle

31 Scopus citations

Abstract

Recently, the High Energy Stereoscopic System (HESS) and other air Cerenkov telescopes have detected a source of TeV γ-rays coincident with the Galactic center. It is not yet clear whether the γ-rays are produced via leptonic or hadronic processes, so it is important to consider possible acceleration sites for the charged particles that produce the γ-rays. One exciting possibility for the origin of these particles is the central black hole, Sgr A*, where the turbulent magnetic fields close to the event horizon can accelerate protons to TeV energies. Using a realistic model of the density distribution in a 6 × 6 × 6 pc cube at the Galactic center, we here calculate the trajectories followed by these TeV protons as they gyrate through the turbulent medium surrounding Sgr A*. Diffusing out from the black hole, the protons produce TeV γ-rays via π° decay following a collision with a proton in the surrounding medium. After following over 222,000 such trajectories, we find that the circumnuclear ring around Sgr A* can reproduce the observed 0.1-100 TeV HESS spectrum and flux if the protons are injected into this medium with an effective power-law index ≈0.75, significantly harder than the observed photon index of 2.25. The total energy in the steady state 1-40 TeV proton population surrounding Sgr A* is inferred to be ≈5 × 1045 ergs. Only 31% of the emitted 1-100 TeV protons encounter the circumnuclear torus, leaving a large flux of protons that diffuse outward to contribute to the Galactic ridge emission observed by HESS on scales of ≳1°

Original languageEnglish (US)
Pages (from-to)L13-L16
JournalAstrophysical Journal
Volume657
Issue number1 II
DOIs
StatePublished - Mar 1 2007

Keywords

  • Acceleration of particles
  • Galaxy: center
  • Gamma rays: theory radiation mechanisms: nonthermal

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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