{ "id": "1103.1002", "version": "v1", "published": "2011-03-05T03:21:05.000Z", "updated": "2011-03-05T03:21:05.000Z", "title": "Origin of the Fermi Bubble", "authors": [ "K. S. Cheng", "D. O. Chernyshov", "V. A. Dogiel", "C. -M. Ko", "W. -H. Ip" ], "comment": "16 pages, 1 figure, accepted for publication in ApJ Letters", "categories": [ "astro-ph.HE" ], "abstract": "Fermi has discovered two giant gamma-ray-emitting bubbles that extend nearly 10kpc in diameter north and south of the galactic center (GC). The existence of the bubbles was first evidenced in X-rays detected by ROSAT and later WMAP detected an excess of radio signals at the location of the gamma-ray bubbles. We propose that periodic star capture processes by the galactic supermassive black hole, Sgr A$^*$, with a capture rate $3\\times 10^{-5}$yr$^{-1}$ and energy release $\\sim 3\\times 10^{52}$erg per capture can produce very hot plasma $\\sim 10$keV with a wind velocity $\\sim 10^8$cm/s injected into the halo and heat up the halo gas to $\\sim 1$keV, which produces thermal X-rays. The periodic injection of hot plasma can produce shocks in the halo and accelerate electrons to $\\sim$TeV, which produce radio emission via synchrotron radiation, and gamma-rays via inverse Compton scattering with the relic and the galactic soft photons.", "revisions": [ { "version": "v1", "updated": "2011-03-05T03:21:05.000Z" } ], "analyses": { "keywords": [ "fermi bubble", "hot plasma", "periodic star capture processes", "produces thermal x-rays", "galactic supermassive black hole" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/731/1/L17", "journal": "The Astrophysical Journal", "year": 2011, "month": "Apr", "volume": 731, "number": 1 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 891652, "adsabs": "2011ApJ...731L..17C" } } }