Journal article · Preprint article
NuSTAR Hard X-ray Survey of the Galactic Center Region. I. Hard X-ray Morphology and Spectroscopy of the Diffuse Emission
Columbia University1
Astrophysics, National Space Institute, Technical University of Denmark2
California Institute of Technology3
ASI Science Data Center4
IT-Department, National Space Institute, Technical University of Denmark5
Hiroshima University6
SLAC National Accelerator Laboratory7
Lawrence Livermore National Laboratory8
NASA Goddard Space Flight Center9
University of California at Berkeley10
Harvard-Smithsonian Center for Astrophysics11
Max Planck Institute for Extraterrestrial Physics12
Pontificia Universidad Católica de Chile13
Durham University14
Massachusetts Institute of Technology15
Université Fédérale Toulouse Midi-Pyrénées16
National Space Institute, Technical University of Denmark17
...and 7 moreWe present the first sub-arcminute images of the Galactic Center above 10 keV, obtained with NuSTAR. NuSTAR resolves the hard X-ray source IGR J17456-2901 into non-thermal X-ray filaments, molecular clouds, point sources, and a previously unknown central component of hard X-ray emission (CHXE). NuSTAR detects four non-thermal X-ray filaments, extending the detection of their power-law spectra with Gamma similar to 1.3-2.3 up to similar to 50 keV.
A morphological and spectral study of the filaments suggests that their origin may be heterogeneous, where previous studies suggested a common origin in young pulsar wind nebulae (PWNe). NuSTAR detects non-thermal X-ray continuum emission spatially correlated with the 6.4 keV Fe K alpha fluorescence line emission associated with two Sgr A molecular clouds: MC1 and the Bridge.
Broadband X-ray spectral analysis with a Monte-Carlo based X-ray reflection model self-consistently determined their intrinsic column density (similar to 10(23) cm(-2)), primary X-ray spectra (power-laws with Gamma similar to 2) and set a lower limit of the X-ray luminosity of Sgr A* flare illuminating the Sgr A clouds to L-X >= 10(38) erg s(-1).
Above similar to 20 keV, hard X-ray emission in the central 10 pc region around Sgr A* consists of the candidate PWN G359.95-0.04 and the CHXE, possibly resulting from an unresolved population of massive CVs with white dwarf masses M-WD similar to 0.9M(circle dot). Spectral energy distribution analysis suggests that G359.95-0.04 is likely the hard X-ray counterpart of the ultra-high gamma-ray source HESS J1745-290, strongly favoring a leptonic origin of the GC TeV emission.
Language: | English |
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Publisher: | American Astronomical Society |
Year: | 2015 |
Pages: | 94 |
ISBN: | 1493966022 , 1493966030 , 9781493966028 and 9781493966035 |
ISSN: | 15384357 and 0004637x |
Types: | Journal article and Preprint article |
DOI: | 10.1088/0004-637x/814/2/94 |
ORCIDs: | 0000-0002-9709-5389 , 0000-0003-2737-5673 , 0000-0002-8686-8737 , 0000-0001-5506-9855 , 0000-0002-5896-6313 , 0000-0002-0393-9190 , Christensen, Finn Erland , 0000-0003-1252-4891 , 0000-0002-8074-4186 , 0000-0002-2734-7835 , 0000-0003-1703-8796 , 0000-0003-2686-9241 , Hornstrup, Allan and Westergaard, Niels J. |