Millenium study of SN 1006 with Suzaku

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

doi:10.1143/PTPS.169.142

Millenium study of SN 1006 with Suzaku

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

^*Corresponding author for this work

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

Abstract

SN 1006 is the milestone of understanding the acceleration mechanism of cosmic rays, and this year is the millennium year for the remnant. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) onboard Suzaku satellite. Thanks to the excellent spectral response of XIS, K emission lines from highly ionized oxygen were clearly resolved. The intensity maps of these lines have been made additional to the intensity and photon index maps of the nonthermal component. We discovered that regions with strong and hard nonthermal component has weak thermal emission. The north rim of the SNR has the hardest nonthermal component. These facts might have information of efficient cosmic ray acceleration and background plasma.

Original language	English
Pages (from-to)	142-145
Number of pages	4
Journal	Progress of Theoretical Physics Supplement
Issue number	169
DOIs	https://doi.org/10.1143/PTPS.169.142
Publication status	Published - 2007
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1143/PTPS.169.142

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Bamba, A., Yamaguchi, H., Koyama, K., Hiraga, J. S., Holt, S., Hughes, J. P., Katagiri, H., Kataoka, J., Kitamoto, S., Kokubun, M., Matumoto, H., Miyata, E., Mori, K., Nakajima, H., Ozaki, M., Petre, R., Sekiguchi, A., Takahashi, T., Tanaka, T., ... Watanabe, S. (2007). Millenium study of SN 1006 with Suzaku. Progress of Theoretical Physics Supplement, (169), 142-145. https://doi.org/10.1143/PTPS.169.142

Bamba, A, Yamaguchi, H, Koyama, K, Hiraga, JS, Holt, S, Hughes, JP, Katagiri, H, Kataoka, J, Kitamoto, S, Kokubun, M, Matumoto, H, Miyata, E, Mori, K, Nakajima, H, Ozaki, M, Petre, R, Sekiguchi, A, Takahashi, T, Tanaka, T, Terada, Y, Tomida, H, Tsunemi, H, Tsuboi, Y, Tsujimoto, M, Uchiyama, Y, Ueno, M & Watanabe, S 2007, 'Millenium study of SN 1006 with Suzaku', Progress of Theoretical Physics Supplement, no. 169, pp. 142-145. https://doi.org/10.1143/PTPS.169.142

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title = "Millenium study of SN 1006 with Suzaku",

abstract = "SN 1006 is the milestone of understanding the acceleration mechanism of cosmic rays, and this year is the millennium year for the remnant. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) onboard Suzaku satellite. Thanks to the excellent spectral response of XIS, K emission lines from highly ionized oxygen were clearly resolved. The intensity maps of these lines have been made additional to the intensity and photon index maps of the nonthermal component. We discovered that regions with strong and hard nonthermal component has weak thermal emission. The north rim of the SNR has the hardest nonthermal component. These facts might have information of efficient cosmic ray acceleration and background plasma.",

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year = "2007",

doi = "10.1143/PTPS.169.142",

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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 - Kitamoto, Shunji

AU - Kokubun, Motohide

AU - Matumoto, Hironori

AU - Miyata, Emi

AU - Mori, Koji

AU - Nakajima, Hiroshi

AU - Ozaki, Masanobu

AU - Petre, Robert

AU - Sekiguchi, Akiko

AU - Takahashi, Tadayuki

AU - Tanaka, Takaaki

AU - Terada, Yukikatsu

AU - Tomida, Hiroshi

AU - Tsunemi, Hiroshi

AU - Tsuboi, Yohko

AU - Tsujimoto, Masahiro

AU - Uchiyama, Yasunobu

AU - Ueno, Masaru

AU - Watanabe, Shin

PY - 2007

Y1 - 2007

N2 - SN 1006 is the milestone of understanding the acceleration mechanism of cosmic rays, and this year is the millennium year for the remnant. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) onboard Suzaku satellite. Thanks to the excellent spectral response of XIS, K emission lines from highly ionized oxygen were clearly resolved. The intensity maps of these lines have been made additional to the intensity and photon index maps of the nonthermal component. We discovered that regions with strong and hard nonthermal component has weak thermal emission. The north rim of the SNR has the hardest nonthermal component. These facts might have information of efficient cosmic ray acceleration and background plasma.

AB - SN 1006 is the milestone of understanding the acceleration mechanism of cosmic rays, and this year is the millennium year for the remnant. We carried out SN 1006 mapping observations with the X-ray Imaging Spectrometers (XIS) onboard Suzaku satellite. Thanks to the excellent spectral response of XIS, K emission lines from highly ionized oxygen were clearly resolved. The intensity maps of these lines have been made additional to the intensity and photon index maps of the nonthermal component. We discovered that regions with strong and hard nonthermal component has weak thermal emission. The north rim of the SNR has the hardest nonthermal component. These facts might have information of efficient cosmic ray acceleration and background plasma.

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JO - Progress of Theoretical Physics Supplement

JF - Progress of Theoretical Physics Supplement

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ER -

Millenium study of SN 1006 with Suzaku

Abstract

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