No X-Ray Excess from the HESS J1741-302 Region except a New Intermediate Polar Candidate
Hideki Uchiyama, Katsuji Koyama, Hironori Matsumoto, Omar Tibolla,, Sarah Kaufmann, Stefan Wagner

TL;DR
This study used Suzaku observations to identify a new intermediate polar candidate near HESS J1741-302, finding no X-ray excess from the gamma-ray source but revealing a magnetized white dwarf binary with characteristic pulsations and iron lines.
Contribution
The paper reports the discovery of a new intermediate polar candidate with specific X-ray spectral features and pulsations, providing insights into the nature of the gamma-ray source region.
Findings
No diffuse or point-like X-ray sources detected from HESS J1741-302's bright emission peak.
Identification of Suzaku J174035.6-301416 as a likely intermediate polar with 432.1 s pulsation.
Detection of iron Kα emission lines indicating a magnetized white dwarf binary.
Abstract
With the Suzaku satellite, we observed an unidentified TeV gamma-ray source HESS J1741302 and its surroundings. No diffuse or point-like X-ray sources are detected from the bright southern emission peak of HESS J1741302. From its neighborhood, we found a new intermediate polar candidate at the position of , which is designated as Suzaku J174035.6301416. The spectrum of Suzaku J174035.6301416 exhibits emission lines at the energy of 6.4, 6.7 and 7.0 keV, which can be assigned as the K lines from neutral, He-like and H-like iron, respectively. A coherent pulsation is found at a period of 432.1 0.1 s. The pulse profile is quasi-sinusoidal in the hard X-ray band (48 keV), but is more complicated in the soft X-ray band (13 keV). The moderate period of pulsation, the energy flux,…
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