Helium star

Results: 65



#Item
1T H E QUASAR 0805 + 046 AS A HELIUM-RICH S H E L L STAR Y . P. V A R S H N I Department of Physics, University of Ottawa, Canada K I N 6N5 (Received 3 July, 1985) Abstract. Within the framework of the plasma-laser star m

T H E QUASAR 0805 + 046 AS A HELIUM-RICH S H E L L STAR Y . P. V A R S H N I Department of Physics, University of Ottawa, Canada K I N 6N5 (Received 3 July, 1985) Abstract. Within the framework of the plasma-laser star m

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Source URL: laserstars.org

Language: English - Date: 2006-08-12 23:19:29
    2THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? The stars are spheres of hot gas. Most of them shine because they are fusing hydrogen into helium in their central parts. In this problem we use concepts of both classica

    THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? The stars are spheres of hot gas. Most of them shine because they are fusing hydrogen into helium in their central parts. In this problem we use concepts of both classica

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    Source URL: www.ipho.org

    Language: English - Date: 2009-10-29 21:21:44
    3Physical parameters of helium-rich subdwarf B stars from spectral energy distributions? A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG. N. Ireland. UK Received 15 JulyAccepted 02 Oct

    Physical parameters of helium-rich subdwarf B stars from spectral energy distributions? A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG. N. Ireland. UK Received 15 JulyAccepted 02 Oct

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    Source URL: star.arm.ac.uk

    Language: English - Date: 2003-10-09 06:43:53
      4Astronomy & Astrophysics manuscript no. Hg223 (DOI: will be inserted by hand later) October 3, 2005 Extreme helium stars: non-LTE matters

      Astronomy & Astrophysics manuscript no. Hg223 (DOI: will be inserted by hand later) October 3, 2005 Extreme helium stars: non-LTE matters

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      Source URL: star.arm.ac.uk

      Language: English - Date: 2006-03-07 11:11:25
        5c ESO 2005  Discovery of pulsation in a helium-rich subdwarf B star A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland, UK

        c ESO 2005  Discovery of pulsation in a helium-rich subdwarf B star A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland, UK

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        Source URL: star.arm.ac.uk

        Language: English - Date: 2006-03-07 11:20:02
          6c ESO 2005  Discovery of pulsation in a helium-rich subdwarf B star A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland, UK

          c ESO 2005  Discovery of pulsation in a helium-rich subdwarf B star A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland, UK

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          Source URL: www.arm.ac.uk

          Language: English - Date: 2006-03-07 11:20:02
            7Physical parameters of helium-rich subdwarf B stars from medium resolution optical spectroscopy? A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG. N. Ireland, UK Received 24 DecemberAc

            Physical parameters of helium-rich subdwarf B stars from medium resolution optical spectroscopy? A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG. N. Ireland, UK Received 24 DecemberAc

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            Source URL: star.arm.ac.uk

            Language: English - Date: 2003-03-26 07:45:48
              8Astronomy & Astrophysics manuscript no. (DOI: will be inserted by hand later) January 29, 2002 Non-linear radial pulsation models for the early-type helium stars

              Astronomy & Astrophysics manuscript no. (DOI: will be inserted by hand later) January 29, 2002 Non-linear radial pulsation models for the early-type helium stars

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              Source URL: star.arm.ac.uk

              Language: English - Date: 2006-03-07 07:51:06
                94 Earth Science PF Activity Report 2010 #28 SiO2 is an archetypal oxide as well as an archetypal glass-forming material, and is also the most abundant

                4 Earth Science PF Activity Report 2010 #28 SiO2 is an archetypal oxide as well as an archetypal glass-forming material, and is also the most abundant

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                Source URL: pfwww.kek.jp

                Language: English - Date: 2012-01-30 19:33:30
                10THE GOVERNORS OF ARMAGH OBSERVATORY AND PLANETARIUM Job Description Job Title: Postdoctoral Research Assistant

                THE GOVERNORS OF ARMAGH OBSERVATORY AND PLANETARIUM Job Description Job Title: Postdoctoral Research Assistant

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                Source URL: star.arm.ac.uk

                Language: English - Date: 2015-02-10 12:17:07