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arXiv · 1409.5790

Multiwavelength study of the northeastern outskirts of the extended TeV source HESS J1809-193

Blagoy Rangelov·Bettina Posselt·Oleg Kargaltsev·George G. Pavlov·Jeremy Hare·Igor Volkov
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Abstract

HESS J1809-193 is an extended TeV gamma-ray source in the Galactic Plane. Multiwavelength observations of the HESS J1809-193 field reveal a complex picture. We present results from three CXO 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 gamma-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 as a dark accelerator - a TeV source without visible counterpart at lower energies.

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Blagoy Rangelov, Bettina Posselt, Oleg Kargaltsev, George G. Pavlov, Jeremy Hare, Igor Volkov. 2014-09-19. Multiwavelength study of the northeastern outskirts of the extended TeV source HESS J1809-193. https://doi.org/10.1088/0004-637x/796/1/34

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