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Astro-E2 Ascent Profile

Turn around. Begin roll mode. Astro-E2 Ascent Profile. (3:25). (5:47). (7:02). (21:47). (3:22). ASTRO E2 が上がり、 XRS が働いたら. (3:20). (3:06). (1:15). 「すざく」と命名. 「すざく」衛星の３検出機器：　 HXD, XRS, XIS. First XRS Spectrum on Orbit ! - 60 mK , 7.0 eV @6.9 keV :World (Universe) Records But !!.

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Astro-E2 Ascent Profile

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  1. Turn around Begin roll mode Astro-E2 Ascent Profile (3:25) (5:47) (7:02) (21:47) (3:22) ASTRO E2が上がり、XRSが働いたら (3:20) (3:06) (1:15) 「すざく」と命名

  2. 「すざく」衛星の３検出機器：　HXD, XRS, XIS

  3. First XRSSpectrum on Orbit ! - 60 mK , 7.0 eV @6.9 keV :World (Universe) Records But !! FWHM = 7.0 eV 55Fe x-rays on cal pixelObtained during contact pass FWHM = 6.4 eV

  4. 星間空間の高エネルギー物理学 Suzaku の科学 Cas A（Ｓuzaku) 高エネルギー 電子の起源 と加速機構 SN1006　（ＡＳＣＡ） α =2.7 α =2.7

  5. Bright/Young SNRs : Hard X-ray Tail All have Γ= 2.7

  6. SN1006 RCW 86 Non-Thermal Shell （α=2.7)vs Hot Plasma Tycho Kepler

  7. downstream upstream 1 10-1 Scale length (pc) 10-2 2 5 10 50 Radius of SNR (pc) The scale length vs. radius R/10 30 Dor C RCW 86 Cas A SN 1006 Tycho R/1000 Kepler The scale length is ~ % of the radius.

  8. Analysis of the SN1006 shell α =2.7 Magnetic Field (microG) Age Limited Diffusive shock accele- ration modelwith nearly perpendicular magnetic field. Age-limited E ~ 30-200 TeV Loss-limited E~ 20-50 TeV Loss Limited Maximum Electron Energy (TeV)

  9. Proton Accelerationand/or Much Higher Energy RXJ1713 is the only shell-typeSNR which INTEGRAL has found someIndicationof hard X-ray emission. α =2.3 (HXD)

  10. Contour 20 cm Color 2-7 keV Chandra G28.6-0.1 kT =0.7 Log(nt) = 10.4 NH = 7.4x1022 α =2.1 XMM-Newton G32.45+0.1 α =1.7 Red 0.5-2 keV Blue 2-7 keV 共にFlatなスペクトル 電子：　< 10-100 TeV あるいは、陽子？

  11. AX J1813-178=1.8 AX J1826-13 = 2.4 AX J1838-065= 1.5 G347.5-0.3 = 2.3 100 TeV 以上の電子 （Synchrotron) or 陽子加速　(p –>π, γ） 宇宙最高エネルギー粒子の起源と加速機構宇宙線発見依頼の最大の謎。 その最近傍の実験室　銀河中心　対消滅線、GeV、TeVガンマ線、特異なＸ線

  12. Hot　Ｇａｓ (108 K) Ｓｇｒ　Ａ　Ｅａｓｔ 10-keV Plasma & Cool Gas + Reflection Origin of the 10 keV Plasma ?Big bang of the BH or Multi-SNe ? Origin of the 6.4 keV-line ?X-ray reflection by the Near-Past Bang of the BH BH 6.4 keV 6.7 keV 6.9 keV Ｃool　Ｇａｓ (10 K) 銀河中心

  13. 巨大ブラックホール 3 2 1 Origin of the Non Thermal Emission ? Cosmic Ray Acceleration Non Thermal X-ray Jets and filaments

  14. Restriction of parameters! known parameters: uu,nrolloff, wu,wd unknown parameters: Emax, Bu, Bd,hu, hd, q A. Age limited case B. Loss limited case tacc = tage < tloss tloss = tacc < tage wu = min {Ku/uu, (Kutcool)1/2} wu = Ku/uu wd = Kd/ud wd = max {udtcool, (Kdtcool)1/2} Both cases, Bd = Bu(cos2q+r2sin2q)1/2 nrolloff ~ BE2 hd < hu

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