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

Hironori Matsumoto, Masaru Ueno, Aya Bamba, Yoshiaki Hyodo, Hideyuki Mori, Hideki Uchiyama, Takeshi Go Tsuru, Katsuji Koyama, Jun Kataoka, Hideaki Katagiri, Tadayuki Takahashi, Junko Hiraga, Shigeo Yamauchi, John P. Hughes, Atsushi Senda, Motohide Kokubun, Takayoshi Kohmura, Frederick S. Porter

Research output: Contribution to journalArticle

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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 ergs-1 cm-2 in the 2-10keV 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.

Original languageEnglish
JournalPublications of the Astronomical Society of Japan
Volume59
Issue number1 SPEC. ISS.
Publication statusPublished - 2007
Externally publishedYes

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particle accelerators
rays
x rays
imaging spectrometers
thermal emission
supernova remnants
erg
halos
spectrometer
dust
scattering
galaxies
particle

Keywords

  • Acceleration of particles
  • X-rays: individual (HESS J1616-508)
  • X-rays: ISM

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Matsumoto, H., Ueno, M., Bamba, A., Hyodo, Y., Mori, H., Uchiyama, H., ... Porter, F. S. (2007). Suzaku observations of HESS J1616-508: Evidence for a dark particle accelerator. Publications of the Astronomical Society of Japan, 59(1 SPEC. ISS.).

Suzaku observations of HESS J1616-508 : Evidence for a dark particle accelerator. / Matsumoto, Hironori; Ueno, Masaru; Bamba, Aya; Hyodo, Yoshiaki; Mori, Hideyuki; Uchiyama, Hideki; Tsuru, Takeshi Go; Koyama, Katsuji; Kataoka, Jun; Katagiri, Hideaki; Takahashi, Tadayuki; Hiraga, Junko; Yamauchi, Shigeo; Hughes, John P.; Senda, Atsushi; Kokubun, Motohide; Kohmura, Takayoshi; Porter, Frederick S.

In: Publications of the Astronomical Society of Japan, Vol. 59, No. 1 SPEC. ISS., 2007.

Research output: Contribution to journalArticle

Matsumoto, H, Ueno, M, Bamba, A, Hyodo, Y, Mori, H, Uchiyama, H, Tsuru, TG, Koyama, K, Kataoka, J, Katagiri, H, Takahashi, T, Hiraga, J, Yamauchi, S, Hughes, JP, Senda, A, Kokubun, M, Kohmura, T & Porter, FS 2007, 'Suzaku observations of HESS J1616-508: Evidence for a dark particle accelerator', Publications of the Astronomical Society of Japan, vol. 59, no. 1 SPEC. ISS..
Matsumoto H, Ueno M, Bamba A, Hyodo Y, Mori H, Uchiyama H et al. Suzaku observations of HESS J1616-508: Evidence for a dark particle accelerator. Publications of the Astronomical Society of Japan. 2007;59(1 SPEC. ISS.).
Matsumoto, Hironori ; Ueno, Masaru ; Bamba, Aya ; Hyodo, Yoshiaki ; Mori, Hideyuki ; Uchiyama, Hideki ; Tsuru, Takeshi Go ; Koyama, Katsuji ; Kataoka, Jun ; Katagiri, Hideaki ; Takahashi, Tadayuki ; Hiraga, Junko ; Yamauchi, Shigeo ; Hughes, John P. ; Senda, Atsushi ; Kokubun, Motohide ; Kohmura, Takayoshi ; Porter, Frederick S. / Suzaku observations of HESS J1616-508 : Evidence for a dark particle accelerator. In: Publications of the Astronomical Society of Japan. 2007 ; Vol. 59, No. 1 SPEC. ISS.
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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 ergs-1 cm-2 in the 2-10keV 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.",
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AU - Matsumoto, Hironori

AU - Ueno, Masaru

AU - Bamba, Aya

AU - Hyodo, Yoshiaki

AU - Mori, Hideyuki

AU - Uchiyama, Hideki

AU - Tsuru, Takeshi Go

AU - Koyama, Katsuji

AU - Kataoka, Jun

AU - Katagiri, Hideaki

AU - Takahashi, Tadayuki

AU - Hiraga, Junko

AU - Yamauchi, Shigeo

AU - Hughes, John P.

AU - Senda, Atsushi

AU - Kokubun, Motohide

AU - Kohmura, Takayoshi

AU - Porter, Frederick S.

PY - 2007

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N2 - 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 ergs-1 cm-2 in the 2-10keV 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.

AB - 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 ergs-1 cm-2 in the 2-10keV 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.

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