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- W3099193118 abstract "HESS J1809−193 is an extended TeV γ-ray source in the Galactic plane. Multiwavelength observations of the HESS J1809−193 field reveal a complex picture. We present results from three Chandra X-Ray Observatory and two Suzaku observations of a region in the northeastern outskirts of HESS J1809–193, where enhanced TeV emission has been reported. Our analysis also includes GeV γ-ray and radio data. One of the X-ray sources in the field is the X-ray binary XTE J1810–189, for which we present the outburst history from multiple observatories and confirm that XTE J1810–189 is a strongly variable type I X-ray burster, which can hardly produce TeV emission. We investigate whether there is any connection between the possible TeV extension of HESS J1809−193 and the sources seen at lower energies. We find that another X-ray binary candidate, Suzaku J1811–1900, and a radio supernova remnant, SNR G11.4−0.1, can hardly be responsible for the putative TeV emission. Our multiwavelength classification of fainter X-ray point sources also does not produce a plausible candidate. We conclude that the northeast extension of HESS J1809−193, if confirmed by deeper observations, can be considered a dark accelerator—a TeV source without a visible counterpart at lower energies." @default.
- W3099193118 created "2020-11-23" @default.
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- W3099193118 date "2014-11-03" @default.
- W3099193118 modified "2023-09-24" @default.
- W3099193118 title "MULTIWAVELENGTH STUDY OF THE NORTHEASTERN OUTSKIRTS OF THE EXTENDED TeV SOURCE HESS J1809–193" @default.
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- W3099193118 doi "https://doi.org/10.1088/0004-637x/796/1/34" @default.
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