Astro-Physics

Results: 813



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121

7. BINARY STARS (ZG: 12; CO: 7, 17) • most stars are members of binary systems or multiple systems (triples, quadruples, quintuplets, ...) 7.1 Classification • visual binaries: see the periodic wobbling of two stars

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

Language: English - Date: 2004-11-23 09:01:42
    122

    Self-gravitating Accretion Disks Tobias Müller, Wilhelm Kley Computational Physics Tübingen Institut für Astronomie und Astrophysik, Auf der Morgenstelle 10C, 72076 Tübingen

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    Source URL: astro.twam.info

    Language: English - Date: 2013-09-13 05:06:33
      123

      THIRD-YEAR ASTROPHYSICS Problem Set: Stellar Structure and Evolution (Dr Ph. Podsiadlowski, Michaelmas TermMeasuring Stellar Parameters. Sirius is a visual binary with a period ofyr. Its measured trigono

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

      Language: English - Date: 2006-10-17 08:39:32
        124

        3. THE PHYSICAL STATE OF THE STELLAR INTERIOR Fundamental assumptions: • Although stars evolve, their properties change so slowly that at any time it is a good approximation to neglect the rate of change of these prope

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

        Language: English - Date: 2004-11-18 06:51:31
          125

          arXiv:astro-phv2 31 MarType Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution1 To Appear in the Astrophysical Journ

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          Source URL: web.physics.ucsb.edu

          Language: English - Date: 2004-07-22 15:08:03
            126

            Physics B3: Astrophysics Stellar Structure and Evolution Dr Ph. Podsiadlowski (www-astro.physics.ox.ac.uk/˜podsi/lec mm03.html) DWB (NAPL), Room 702, Tel.: (

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

            Language: English - Date: 2006-10-17 08:38:54
              127

              Ini$al  Development  and  Pilot  Study  Design  of     Interac$ve  Lecture  Demonstra$ons  for  ASTRO  101   Schwortz,  Andria  C.;  French,  Debbie  A.;  Gu$er

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              Source URL: physics.uwyo.edu

              Language: English - Date: 2014-06-03 22:40:47
                128

                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 06:57:38
                  129

                  Magnetohydrodynamics — Historical Evolution and Trends S. Molokov, R. Moreau and H. K. Moffatt, Eds. (Berlin: Springerpp. 85–115 [E-print: astro-phTurbulence and Magnetic Fields in Astrophysical Plas

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

                  Language: English - Date: 2008-12-03 13:51:23
                    130

                    Infrared Signature of Active Massive Black Holes in Nearby Dwarf Galaxies Francine Marleau1, Dominic Clancy1, Matteo Bianconi1, Rebecca Habas1 1 Institute of Astro and Particle Physics, Innsbruck, Austria Central massive

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                    Source URL: events.kuoni-dmc.com

                    Language: English - Date: 2015-03-19 11:47:43
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