Origin of nonthermal emission from the Fermi bubbles and mechanisms of particle acceleration there

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题名:	Origin of nonthermal emission from the Fermi bubbles and mechanisms of particle acceleration there
作者:	高仲明;Dogiel, V. A.;Cheng, K.-S.;Chernyshov, D. O.;Ko, C.-M.
贡献者:	理學院天文研究所
关键词:	Astronomy;Astrophysics;Black holes;Bubbles;Contributed Papers;Particle accelerators;Plasma;Supernovae
日期:	2014-01-01
上传时间:	2026-04-21 14:24:22 (UTC+8)
出版者:	Cambridge University Press;Cambridge, UK: Cambridge University Press
摘要:	摘要： The discovery of the two giant γ-ray lobes (Fermi bubbles) in the Galactic center (see Dobler et al. 2010 and Su et al. 2010) was one of the most impressive events of the last few years in astrophysics. However, some indications on giant structures in the Galactic center (GC) were observed several years before by WMAP in the radio frequency range between 23 and 33 MHz (Finkbeiner 2004), and by ROSAT in hard X-rays (Bland-Hawthorn & Cohen 2003). Recent observations performed by the Planck Collaboration (Ade et al. 2012) found also lobes in the microwave range which spatially coincided the Fermi bubbles that indicated on the common origin of these phenomena. 其他題名： Proc. IAU 出版者： Cambridge, UK: Cambridge University Press 出版日期： 2013-10-01 出處： Proceedings of the International Astronomical Union, 2013-10, Vol.9 (S303), p.399-402 資源來源： Alma/SFX Local Collection 版權： Copyright © International Astronomical Union 2014 識別號： ISSN: 1743-9213 識別號： ISSN: 1743-9221 識別號： EISSN: 1743-9221 識別號： DOI: 10.1017/S174392131400101X
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