Suzaku observations of HESS J1616-508 : Evidence for a dark particle accelerator
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Abstract
We observed the bright unidentified TeV γ -ray source HESS J1616-508 with the X-ray Imaging Spectrometers onboard the Suzaku satellite. No X-ray counterpart was found to a limiting flux of 3.1 × 10-13 erg s-1 cm-2 in the 2–10 keV band, which is some 60-times below the γ -ray flux in the 1–10 TeV band. This object is bright in TeV γ -rays, but very dim in the X-ray band, and thus is one of the best examples in the Galaxy of a “dark particle accelerator." We also detected soft thermal emission with kT ∼ 0.3–0.6keV near the location of HESS J1616-508. This may be due to a dust-grain scattering halo from the nearby bright supernova remnant RCW 103.
Journal
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- Publications of the Astronomical Society of Japan
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Publications of the Astronomical Society of Japan 59 S199-S208, 2007-01-25
日本天文学会
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Details 詳細情報について
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- CRID
- 1050577740963891584
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- NII Article ID
- 10023948831
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- NII Book ID
- AA1082896X
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- ISSN
- 00046264
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- NDL BIB ID
- 8621309
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- Text Lang
- en
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- Article Type
- journal article
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- Data Source
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- IRDB
- NDL
- CiNii Articles
- KAKEN