Origin of the Fermi bubble

K. S. Cheng, D. O. Chernyshov, V. A. Dogiel, C. M. Ko, W. H. Ip

研究成果: 雜誌貢獻期刊論文同行評審

95 引文 斯高帕斯(Scopus)

摘要

Fermi has discovered two giant gamma-ray-emitting bubbles that extend nearly 10kpc in diameter north and south of the Galactic center. 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 × 10-5 yr -1 and energy release ∼3 × 1052 erg per capture can produce very hot plasma ∼10 keV with a wind velocity ∼108 cm s-1 injected into the halo and heat up the halo gas to ∼1 keV, which produces thermal X-rays. The periodic injection of hot plasma can produce shocks in the halo and accelerate electrons to ∼TeV, which produce radio emission via synchrotron radiation and gamma rays via inverse Compton scattering with the relic and the galactic soft photons.

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文章編號L17
期刊Astrophysical Journal Letters
731
發行號1 PART II
DOIs
出版狀態已出版 - 10 4月 2011

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