Oxygen line mapping of SN 1006 with Suzaku

Aya Bamba; Hiroya Yamaguchi; Katsuji Koyama; Junko S. Hiraga; Steve Holt; John P. Hughes; Hideaki Katagiri; Jun Kataoka; Satoru Katsuda; Shunji Kitamoto; Motohide Kokubun; Hironori Matsumoto; Emi Miyata; Koji Mori; Hiroshi Nakajima; Masanobu Ozaki; Rob Petre; Akiko Sekiguchi; Tadayuki Takahashi; Takaaki Tanaka; Yukikatsu Terada; Hiroshi Tomida; Yohko Tsuboi; Masahiro Tsujimoto; Hiroshi Tsunemi; Yasunobu Uchiyama; Masaru Ueno; Shin Watanabe

doi:10.1016/j.asr.2007.03.055

Oxygen line mapping of SN 1006 with Suzaku

Aya Bamba, Hiroya Yamaguchi, Katsuji Koyama, Junko S. Hiraga, Steve Holt, John P. Hughes, Hideaki Katagiri, Jun Kataoka, Satoru Katsuda, Shunji Kitamoto, Motohide Kokubun, Hironori Matsumoto, Emi Miyata, Koji Mori, Hiroshi Nakajima, Masanobu Ozaki, Rob Petre, Akiko Sekiguchi, Tadayuki Takahashi, Takaaki TanakaYukikatsu Terada, Hiroshi Tomida, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Yasunobu Uchiyama, Masaru Ueno, Shin Watanabe

Research output: Contribution to journal › Article › peer-review

3 Citations (Scopus)

Abstract

SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region.

Original language	English
Pages (from-to)	411-415
Number of pages	5
Journal	Advances in Space Research
Volume	41
Issue number	3
DOIs	https://doi.org/10.1016/j.asr.2007.03.055
Publication status	Published - 2008
Externally published	Yes

Keywords

Acceleration of particles
ISM: individual (SN 1006)
X-rays: ISM

ASJC Scopus subject areas

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
Earth and Planetary Sciences(all)

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Bamba, A., Yamaguchi, H., Koyama, K., Hiraga, J. S., Holt, S., Hughes, J. P., Katagiri, H., Kataoka, J., Katsuda, S., Kitamoto, S., Kokubun, M., Matsumoto, H., Miyata, E., Mori, K., Nakajima, H., Ozaki, M., Petre, R., Sekiguchi, A., Takahashi, T., ... Watanabe, S. (2008). Oxygen line mapping of SN 1006 with Suzaku. Advances in Space Research, 41(3), 411-415. https://doi.org/10.1016/j.asr.2007.03.055

Oxygen line mapping of SN 1006 with Suzaku. / Bamba, Aya; Yamaguchi, Hiroya; Koyama, Katsuji; Hiraga, Junko S.; Holt, Steve; Hughes, John P.; Katagiri, Hideaki; Kataoka, Jun; Katsuda, Satoru; Kitamoto, Shunji; Kokubun, Motohide; Matsumoto, Hironori; Miyata, Emi; Mori, Koji; Nakajima, Hiroshi; Ozaki, Masanobu; Petre, Rob; Sekiguchi, Akiko; Takahashi, Tadayuki; Tanaka, Takaaki; Terada, Yukikatsu; Tomida, Hiroshi; Tsuboi, Yohko; Tsujimoto, Masahiro; Tsunemi, Hiroshi; Uchiyama, Yasunobu; Ueno, Masaru; Watanabe, Shin.

In: Advances in Space Research, Vol. 41, No. 3, 2008, p. 411-415.

Research output: Contribution to journal › Article › peer-review

Bamba, A, Yamaguchi, H, Koyama, K, Hiraga, JS, Holt, S, Hughes, JP, Katagiri, H, Kataoka, J, Katsuda, S, Kitamoto, S, Kokubun, M, Matsumoto, H, Miyata, E, Mori, K, Nakajima, H, Ozaki, M, Petre, R, Sekiguchi, A, Takahashi, T, Tanaka, T, Terada, Y, Tomida, H, Tsuboi, Y, Tsujimoto, M, Tsunemi, H, Uchiyama, Y, Ueno, M & Watanabe, S 2008, 'Oxygen line mapping of SN 1006 with Suzaku', Advances in Space Research, vol. 41, no. 3, pp. 411-415. https://doi.org/10.1016/j.asr.2007.03.055

Bamba, Aya ; Yamaguchi, Hiroya ; Koyama, Katsuji ; Hiraga, Junko S. ; Holt, Steve ; Hughes, John P. ; Katagiri, Hideaki ; Kataoka, Jun ; Katsuda, Satoru ; Kitamoto, Shunji ; Kokubun, Motohide ; Matsumoto, Hironori ; Miyata, Emi ; Mori, Koji ; Nakajima, Hiroshi ; Ozaki, Masanobu ; Petre, Rob ; Sekiguchi, Akiko ; Takahashi, Tadayuki ; Tanaka, Takaaki ; Terada, Yukikatsu ; Tomida, Hiroshi ; Tsuboi, Yohko ; Tsujimoto, Masahiro ; Tsunemi, Hiroshi ; Uchiyama, Yasunobu ; Ueno, Masaru ; Watanabe, Shin. / Oxygen line mapping of SN 1006 with Suzaku. In: Advances in Space Research. 2008 ; Vol. 41, No. 3. pp. 411-415.

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abstract = "SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region.",

keywords = "Acceleration of particles, ISM: individual (SN 1006), X-rays: ISM",

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T1 - Oxygen line mapping of SN 1006 with Suzaku

AU - Bamba, Aya

AU - Yamaguchi, Hiroya

AU - Koyama, Katsuji

AU - Hiraga, Junko S.

AU - Holt, Steve

AU - Hughes, John P.

AU - Katagiri, Hideaki

AU - Kataoka, Jun

AU - Katsuda, Satoru

AU - Kitamoto, Shunji

AU - Kokubun, Motohide

AU - Matsumoto, Hironori

AU - Miyata, Emi

AU - Mori, Koji

AU - Nakajima, Hiroshi

AU - Ozaki, Masanobu

AU - Petre, Rob

AU - Sekiguchi, Akiko

AU - Takahashi, Tadayuki

AU - Tanaka, Takaaki

AU - Terada, Yukikatsu

AU - Tomida, Hiroshi

AU - Tsuboi, Yohko

AU - Tsujimoto, Masahiro

AU - Tsunemi, Hiroshi

AU - Uchiyama, Yasunobu

AU - Ueno, Masaru

AU - Watanabe, Shin

PY - 2008

Y1 - 2008

N2 - SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region.

AB - SN 1006 is one of the supernova remnants (SNRs) with relatively low-temperature electrons, considering the young age of just 1000 years. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) and the Hard X-ray Detector (HXD) onboard Suzaku, the fifth Japanese X-ray satellite. Thanks to the excellent spectral resolution of XIS in the soft X-ray band, H-like and He-like oxygen emission lines were clearly detected, and we could make a map of the line intensity, and as well as a flux and the photon index of nonthermal component. We found that these parameters have spatial dependences from region to region in the SNR; the north region is bright in nonthermal, while dim in thermal; the east region is bright in both nonthermal and thermal; the inner region shows dim nonthermal and bright thermal emission. The photon index is the smallest in the north region.

KW - Acceleration of particles

KW - ISM: individual (SN 1006)

KW - X-rays: ISM

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