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X-Ray and Gamma-Ray Emission from the Galactic Center

V. A. Dogiel K. -S. Cheng D. O. Chernyshov W. -H. Ip C. -M. Ko V. Tatischeff 1
1 CSNSM AN
CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
Abstract : We discuss the origin of continuum and line X-ray emission observed in the direction the Galactic Center. We predict a significant flux of de-excitation gamma-ray lines in this direction, which can be produced by subrelativistic protons generated by accretion processes.
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Conference papers
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http://hal.in2p3.fr/in2p3-00650704
Contributor : Christine Hadrossek Connect in order to contact the contributor
Submitted on : Monday, December 12, 2011 - 10:09:04 AM
Last modification on : Wednesday, September 16, 2020 - 5:38:34 PM

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  • HAL Id : in2p3-00650704, version 1
  • ARXIV : 1002.1379

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V. A. Dogiel, K. -S. Cheng, D. O. Chernyshov, W. -H. Ip, C. -M. Ko, et al.. X-Ray and Gamma-Ray Emission from the Galactic Center. Conference on the Galactic Center: A Window to the Nuclear Environment of Disk Galaxies, Oct 2009, Shangai, China. pp.426. ⟨in2p3-00650704⟩

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