Stellar structure

Results: 127



#Item
1Reddening structure and metallicities of the Milky Way Bulge from VVV and 2MASS Oscar A. Gonzalez European Southern Observatory Optical and Infrared Galactic Plane surveys – University of Hertfordshire – July 2011

Reddening structure and metallicities of the Milky Way Bulge from VVV and 2MASS Oscar A. Gonzalez European Southern Observatory Optical and Infrared Galactic Plane surveys – University of Hertfordshire – July 2011

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Source URL: star.herts.ac.uk

Language: English - Date: 2011-08-16 06:23:10
2The After SDSS-IV, Letter of Intent: Andrew Tkachenko on behalf of the KU Leuven Gaia/K2/TESS/PLATO2.0 team (Institute of Astronomy, KU Leuven, Belgium) Constraining the theories of stellar structure and evolution throug

The After SDSS-IV, Letter of Intent: Andrew Tkachenko on behalf of the KU Leuven Gaia/K2/TESS/PLATO2.0 team (Institute of Astronomy, KU Leuven, Belgium) Constraining the theories of stellar structure and evolution throug

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Source URL: www.sdss.org

Language: English - Date: 2016-07-30 19:27:59
3Characterizing the Structure of Embedded Clusters with the Spitzer Young Stellar Clusters Survey Rob Gutermuth: Harvard-Smithsonian Center for Astrophysics Phil Myers, CfA

Characterizing the Structure of Embedded Clusters with the Spitzer Young Stellar Clusters Survey Rob Gutermuth: Harvard-Smithsonian Center for Astrophysics Phil Myers, CfA

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Source URL: conference.astro.ufl.edu

Language: English - Date: 2007-04-20 10:38:33
    4STELLAR 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])

    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
      5Physics 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.

      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
        6STRUCTURE OF THE SUN HELIOSEISMOLOGY (I) • The Sun is the only star for which we can measure internal properties → test of stellar structure theory

        STRUCTURE OF THE SUN HELIOSEISMOLOGY (I) • The Sun is the only star for which we can measure internal properties → test of stellar structure theory

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

        Language: English - Date: 2003-10-31 06:50:52
          7Page 2 Stellar Structure and Evolution: Syllabus Ph. Podsiadlowski (MTDWB 702, (, ) (www-astro.physics.ox.ac.uk/˜podsi/lec mm03.html)

          Page 2 Stellar Structure and Evolution: Syllabus Ph. Podsiadlowski (MTDWB 702, (, ) (www-astro.physics.ox.ac.uk/˜podsi/lec mm03.html)

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

          Language: English - Date: 2006-10-17 08:40:36
            8STELLAR 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])

            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 05:30:04
              9STRUCTURE OF THE SUN HELIOSEISMOLOGY (I) • The Sun is the only star for which we can measure internal properties → test of stellar structure theory

              STRUCTURE OF THE SUN HELIOSEISMOLOGY (I) • The Sun is the only star for which we can measure internal properties → test of stellar structure theory

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

              Language: English - Date: 2003-10-31 06:50:58
                10THIRD-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

                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