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20062008
most citedA Testable the Stochastic Acceleration Model for Flares in Sagittarius A*

43 citations

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astro-ph200810 cited

Modulated X-ray Emissivity near the Stress Edge in Sgr A*

M. Falanga, F. Melia, M. Prescher +2

Sgr A* is thought to be the radiative manifestation of a ~3.6E6 Msun supermassive black hole at the Galactic center. Its mm/sub-mm spectrum and its flare emission at IR and X-ray w…

astro-ph20076 cited

Radio Synchrotron Emission from Secondary Leptons in the Vicinity of Sgr A*

Roland M. Crocker, David Jones, David R. Ballantyne +1

A point-like source of ~TeV gamma-rays has recently been seen towards the Galactic center by HESS and other air Cerenkov telescopes. In recent work (Ballantyne et al. 2007), we dem…

astro-ph200741 cited

General Relativistic Flux Modulations from Disk Instabilities in Sagittarius A*

Maurizio Falanga, Fulvio Melia, Michel Tagger +2

Near-IR and X-ray flares have been detected from the supermassive black hole Sgr A* at the center of our Galaxy with a (quasi)-period of ~17-20 minutes, suggesting an emission regi…

astro-ph200730 cited

A Possible Link Between the Galactic Center HESS Source and Sgr A*

D. R. Ballantyne, Fulvio Melia, Siming Liu +1

Recently, HESS and other air Cerenkov telescopes have detected a source of TeV gamma-rays coincident with the Galactic center. It is not yet clear whether the gamma-rays are produc…

astro-ph200643 cited

A Testable the Stochastic Acceleration Model for Flares in Sagittarius A*

Siming Liu, Vahe Petrosian, Fulvio Melia +1

The near-IR and X-ray flares in Sagittarius A* are believed to be produced by relativistic electrons via synchrotron and synchrotron self-Comptonization, respectively. These electr…