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    Fare clic per modificare stileFare clic per modificare gli stili del testo dello schemaSecondo livelloTerzo livelloQuarto livelloQuinto livelloWIMP dark matter starsFabio IoccoInstitut de Physique Th

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    マスター タイトルの書式設定マスター テキストの書式設定第 2 レベル第 3 レベル第 4 レベル第 5 レベルExcesses of Magnetic Flux and Angular Momentum in StarsNational Astronomical Observatory (NAOJ)Kohji Tomisaka Angular MomentumAngular Momentum P

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  • ASTR1101001Spring2008.ppt

    Click to edit Master title styleClick to edit Master text stylesSecond levelThird levelFourth levelFifth levelASTR 1101-001Spring 2008Joel E. Tohline Alumni Professor247 Nicholson Hall[Slides from Lec

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  • ...AtAstrophysicalShocksImplicationsfTheiginof.ppt

    Particle Acceleration At Astrophysical ShocksAnd Implications for The Origin of Cosmic RaysPasquale BlasiArcetri Astrophysical Observatory Firenze - Italy INAFNational Institute for Astrophysi

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  • ASTR1101001Spring2008.ppt

    Click to edit Master title styleClick to edit Master text stylesSecond levelThird levelFourth levelFifth levelASTR 1101-001Spring 2008Joel E. Tohline Alumni Professor247 Nicholson Hall[Slides from Lec

    日期:2022-04-22 格式:.pptx 页数:28页 大小:1.09MB 发布:
  • DiskevolutionClearing.ppt

    Disk evolution and ClearingP. DAlessio (CRYA)C. Briceno (CIDA)J. Hernandez (CIDA Michigan)L. Hartmann (Michigan)J. Muzerolle (Steward)A. Sicilia-Aguilar (Heidelberg)SpitzerIRS disk modeling teamL.

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  • CosmicRaysGalacticField.ppt

    Click to edit Master title styleClick to edit Master text stylesSecond levelThird levelFourth levelFifth levelCosmic Rays and Galactic Field3 March 2003Astronomy G9001 - Spring 2003Prof. Mordecai-Mark

    日期:2022-04-22 格式:.pptx 页数:43页 大小:529KB 发布:
  • Gammarayburstsfrombinaryblackholes.ppt

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  • ResonanceCaptureWhendoesitHappen.ppt

    Resonance Capture When does it HappenAlice Quillen University of RochesterDepartment of Physics and AstronomyResonance CaptureAstrophysical Settings Migrating planets moving inward or outward capt

    日期:2022-04-25 格式:.pptx 页数:15页 大小:645KB 发布:
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