Helium-3

Results: 331



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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
    2Magnetic Resonance in Medicine 63:41–Helium-3 MR q-Space Imaging With Radial Acquisition and Iterative Highly Constrained Back-Projection Rafael L. O’Halloran,1 James H. Holmes,1 Yu-Chien Wu,2,3 Andrew Ale

    Magnetic Resonance in Medicine 63:41–Helium-3 MR q-Space Imaging With Radial Acquisition and Iterative Highly Constrained Back-Projection Rafael L. O’Halloran,1 James H. Holmes,1 Yu-Chien Wu,2,3 Andrew Ale

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    Source URL: haxbylab.dartmouth.edu

    - Date: 2016-08-01 11:09:14
      3Is There a Better Route to Fusion? Todd H. Rider  April 1, 2005 “Thirty-five years ago I was an expert precious-metal quartz-miner. There was an outcrop in my neighborhood that assayed $600 a ton—gol

      Is There a Better Route to Fusion? Todd H. Rider April 1, 2005 “Thirty-five years ago I was an expert precious-metal quartz-miner. There was an outcrop in my neighborhood that assayed $600 a ton—gol

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      Source URL: www.longwood.edu

      Language: English - Date: 2009-03-03 13:31:30
      4By Eugene F. Mallove, Sc.D.  BREAKING THROUGH WELCOME ICCF-7! — Seeing the “Big Picture”

      By Eugene F. Mallove, Sc.D. BREAKING THROUGH WELCOME ICCF-7! — Seeing the “Big Picture”

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      Source URL: www.infinite-energy.com

      Language: English - Date: 2014-07-09 11:50:02
      5#26 QUARK _  #26 QUARK in progress

      #26 QUARK _ #26 QUARK in progress

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      Source URL: www.infinite-energy.com

      Language: English - Date: 2014-07-09 14:14:00
      6THEORETICAL 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
      7letters to nature  Upper-mantle dynamics revealed by helium isotope variations along the southeast Indian ridge D. W. Graham*, J. E. Lupton², F. J. Spera³ & D. M. Christie*

      letters to nature Upper-mantle dynamics revealed by helium isotope variations along the southeast Indian ridge D. W. Graham*, J. E. Lupton², F. J. Spera³ & D. M. Christie*

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      Source URL: noblegaslab.coas.oregonstate.edu

      Language: English - Date: 2001-02-12 14:36:58
      8AKARI Observer’s Manual for the Post-Helium (Phase 3) Mission Version 1.2  — for Open Time Observation Planning —

      AKARI Observer’s Manual for the Post-Helium (Phase 3) Mission Version 1.2 — for Open Time Observation Planning —

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      Source URL: www.ir.isas.jaxa.jp

      Language: English - Date: 2009-05-21 20:59:04
        9Astronomy & 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
          10Astronomy & 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: www.arm.ac.uk

          Language: English - Date: 2006-03-07 11:11:25