Diffuse X-rays in the Galactic center region -- The zoo of iron line clumps, non-thermal filaments and hot plasmas --

Aya Bamba; Hiroshi Murakami; Atsushi Senda; Shin-ichiro Takagi; Jun Yokogawa; Katsuji Koyama

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Diffuse X-rays in the Galactic center region -- The zoo of iron line clumps, non-thermal filaments and hot plasmas --

Aya Bamba·Hiroshi Murakami·Atsushi Senda·Shin-ichiro Takagi·Jun Yokogawa·Katsuji Koyama

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Abstract

This paper reports the diffuse X-ray features around the Galactic center observed with Chandra. We confirm the ASCA and Ginga discoveries of the large-scale thin-thermal plasma with strong lines in the Galactic center region. In addition, many small clumps of emission lines from neutral (6.4 keV line) to He-like (6.7 keV line) irons are discovered. The 6.4 keV line clumps would be reflection nebulae, while those of the 6.7 keV line are likely SNRs. We also find emission lines of intermediate energy between 6.5-6.7 keV, which are attributable to young SNRs in non equilibrium ionization. Non-thermal filaments or belts with X-ray spectra of no emission line are found, suggesting the Fermi acceleration site in a rapidly expanding shell. All these suggest that multiple-supernovae or extremely large explosion had occurred around the Galactic center region in the recent past.

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Aya Bamba, Hiroshi Murakami, Atsushi Senda, Shin-ichiro Takagi, Jun Yokogawa, Katsuji Koyama. 2002-02-01. Diffuse X-rays in the Galactic center region -- The zoo of iron line clumps, non-thermal filaments and hot plasmas --. https://arxiv.org/abs/astro-ph/0202010

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