X-ray Threads and Diffuse Emission in the Central 300 pc of the Galaxy

Details X-ray Threads and Diffuse Emission in the Central 300 pc of the Galaxy X-ray Threads and Diffuse Emission in the Central 300 pc of the Galaxy

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.0604l&link_type=abstract

American Astronomical Society, HEAD meeting #7, #06.04; Bulletin of the American Astronomical Society, Vol. 35, p.608

Astronomy and Astrophysics

Astronomy

Scientific paper

We present X-ray spectral and spatial analysis of several filamentary and diffuse features that were first identified in the Chandra Galactic Center Survey. This 300-ks survey covers the central 300 pc of the Galaxy in the energy range of 2-10 keV. These features include the X-ray threads G0.13-0.11, G359.89-0.08, G359.54+0.18, and the diffuse 6.4 keV emission in and around the Arches stellar cluster. These X-ray sources all have radio counterparts and we will present multi-wavelength analysis and discussion of the physical nature of these unique Galactic center objects.

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