Suzaku observations of HESS J1616-508 : Evidence for a dark particle accelerator

Publications of the Astronomical Society of Japan Volume 59 Page S199-S208 published_at 2007-01-25
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Title ( eng )
Suzaku observations of HESS J1616-508 : Evidence for a dark particle accelerator
Creator
Matsumoto Hironori
Ueno Masaru
Bamba Aya
Hyodo Yoshiaki
Mori Hideyuki
Uchiyama Hideki
Tsuru Takeshi Go
Koyama Katsuji
Kataoka Jun
Takahashi Tadayuki
Hiraga Junko
Yamauchi Shigeo
Hughes John P.
Senda Atsushi
Kokubun Motohide
Kohmura Takayoshi
Porter Frederick S.
Source Title
Publications of the Astronomical Society of Japan
Volume 59
Start Page S199
End Page S208
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.
Keywords
acceleration of particles —X-rays: individual (HESS J1616-508) —X-rays: ISM
NDC
Astronomy. Space sciences [ 440 ]
Language
eng
Resource Type journal article
Publisher
日本天文学会
Date of Issued 2007-01-25
Rights
Copyright (c) 2007 Astronomical Society of Japan
Publish Type Version of Record
Access Rights open access
Source Identifier
[ISSN] 0004-6264
[NCID] AA1082896X
[URI] http://pasj.asj.or.jp/v59/sp1/59s115/59s115a.html