The Suzaku Results of SN1006 Koyama, Ｋ. 1, Bamba, A. 2, Yamaguchi, H. 1 1 Kyoto University, 2 Rikken Nickname Suzaku Ancient Oriental mythology ASTRO E2 Launch: 2005/7/10

３ Main Detectors ： HXD, XRS, XIS

E XIS Suzaku XIS-FI Suzaku XIS-BI O VII O VIII Ne IX Ne X Ｇｏｏｄ Response of low energy Low and Stable BG at high energy Galactic Center

Japanese historical record of SNR “Meigetsuki” (This page was written in 11/8, 1230.) 「客星古現例」 the ancient samples of “guest stars”. Guest stars = comets, novae, and supernovae ＜ chronological order SN1006 3C58 Crab Nebula

3C58 Chandra image of 3C58 高倉院 治承五年 六月廿五日 庚午 戌時 客星見北方 近王良 守伝舎星 In the reign-period of Takakura-In, June 25th, 5th year of Jisyou (= August 7th, 1181), a guest star appeared in northern sky at 20:00. It was near to the star of “Oh-Ryo” (= real person’s name of ancient China) and “Densya”. 王良 (Oh-Ryo) Cassiopeiaβ 伝舎 (Densya) = Camelopardalis

Crab nebula Chandra image of Crab 後冷泉院 天喜二年 四月中旬以降 丑時 客星觜参度 見東方 孛天関星 大如歳星 In the reign-period of Goreizei-In, after the middle of April, 2nd year of Tenki (= May-June, 1054), a guest star appeared nearby “Shi” and “Shin” (= Orion) in eastern sky at 2:00. It shined near to the star of “Tenkan”, and its size was comparable to Jupiter. 觜, 参 = Orion 天関 (Tenkan) Taurusζ

SN1006 Chandra image of SN1006 一條院 寛弘三年 四月二日 葵酉 夜以降 騎官中 有大客星 如螢惑 光明動耀 連夜正見南方 或云 騎陣将軍星本体 増変光 In the reign-period of Ichijo-In, April 2nd, 3rd year of Kanko (= May 1st, 1006), a great guest star appeared within the constellation “Kikan” (=Imperial Guards). It was very bright like Mars, and visible in the southern sky every night. 騎陣将軍 (Kijin-Shogun) Lupusκ 騎官 (kikan)

Narrow band images of XIS-BI He-O line band keV band Distributions of thermal plasma (line emission) and non-thermal electron (synchrotron emission) are different !

Black : XIS-BI Red : average of 3 XIS-FIs He-O H-O Non-thermal emission keV band 3-5 keVOVII band See also Poster E

North rim East rim Inner

H-O He-O North rim East rim Inner region H-O/He-O ～ 0.2 in all regions ! Line intensity: East rim > North rim → Density: East rim > North rim H-O/He-O ratio: East rim < North rim → Temperature: East rim < North rim ＣＩＥ Ｐｌａｓｍａ

He-O line vs. hard X-ray emission North rim East rim Inner region Consistent with imaging analysis !

Ｃｈａｎｄｒａ Ｉｍａｇｅ North Rim East Rim

Red ： North Black ： East

North Rim East Rim

SN 1006: Non-Thermal Filaments (Bamba et al.)

(Preliminary) Results North Rim Low density High temp and Highly NEI Flat Γ Sharp W u East Rim High density Low temp and Moderate NEI Steep Γ Slow W u Acceleration efficiency vs Plasma Temp.

朱雀 Suzaku The wall painting of “Suzaku” ｉ n the ancient tomb “Kitora” built in the Asuka Era Southern Sky from Kyoto in AD1006/5/1