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

Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/101110

Title:	Origin of nonthermal emission from the Fermi bubbles and mechanisms of particle acceleration there
Authors:	高仲明;Dogiel, V. A.;Cheng, K.-S.;Chernyshov, D. O.;Ko, C.-M.
Contributors:	理學院天文研究所
Keywords:	Astronomy;Astrophysics;Black holes;Bubbles;Contributed Papers;Particle accelerators;Plasma;Supernovae
Date:	2014-01-01
Issue Date:	2026-04-21 14:24:22 (UTC+8)
Publisher:	Cambridge University Press;Cambridge, UK: Cambridge University Press
Abstract:	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
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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