Astro-Physics

Results: 813



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91

arXiv:1502.03249v1 [astro-ph.IM] 11 FebSignificance in Gamma Ray Astronomy with Systematic Errors Gerrit Spengler1 Oscar Klein Centre for Cosmoparticle Physics, Physics Department, Stockholm University,

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Source URL: arxiv.org

Language: English - Date: 2015-02-11 20:31:29
    92

    Microsoft PowerPoint - campus_map

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    Source URL: astro.physics.brown.edu

    - Date: 2007-10-16 15:41:18
      93

      «ETTORE MAJORANA» FOUNDATION AND CENTRE FOR SCIENTIFIC CULTURE INTERNATIONAL SCHOOLS OF COSMIC-RAY ASTROPHYSICS: ! Progress and Problems in Cosmic Ray Physics ! Acceleration of Particles in Nature ! Comp

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      Source URL: particle.astro.ru.nl

      Language: English - Date: 2015-07-27 11:11:56
        94

        PDF Document

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        Source URL: www.astro-physics.com

        Language: English - Date: 2013-04-10 09:06:23
          95

          APPENDICES (Supplementary Material) A. Brown Dwarfs B. Planets C. The CNO Tri-Cycle D. The Structure of the Sun and the Solar Neutrino Problem

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          Source URL: www-astro.physics.ox.ac.uk

          Language: English - Date: 2004-12-01 08:11:42
            96

            Evolution of protoplanetary disks in binary stars Tobias Müller, Wilhelm Kley Computational Physics Tübingen

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            Source URL: astro.twam.info

            Language: English - Date: 2013-09-13 05:06:54
              97

              Hertzsprung-Russell (Colour-Magnitude) Diagram 2. Correlations between Stellar Properties 2.1 Mass-luminosity relationship (ZG: 12.2; CO: 7.3) • Most stars obey Ls = constant × Ms

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              Source URL: www-astro.physics.ox.ac.uk

              Language: English - Date: 2004-11-18 06:49:38
                98

                5. NUCLEAR REACTIONS (ZG: P5-7 to P5-9, P5-12, 16-1D; CO: 10.3) • Binding energy of nucleus with Z protons and N neutrons is: Q(Z, N) = [ZMp + NMn − M(Z, N)] c2. |

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                Source URL: www-astro.physics.ox.ac.uk

                Language: English - Date: 2004-11-18 06:57:56
                  99

                  STELLAR STRUCTURE AND EVOLUTION 1. OBSERVABLE PROPERTIES OF STARS Basic large-scale observable properties: 1.1 LUMINOSITY (ZG: 11; CO: 3.1) (‘power’, [J/s=W])

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                  Source URL: www-astro.physics.ox.ac.uk

                  Language: English - Date: 2004-11-08 05:27:34
                    100

                    Physics B3: Astrophysics Stellar Structure and Evolution Finals’ Paper: • Exam material is the material covered in the main part of the lectures and has not been marked as supplementary (i.e. not the appendices; e.g.

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                    Source URL: www-astro.physics.ox.ac.uk

                    - Date: 2006-11-03 04:12:12
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