Dark matter halo

Results: 54



#Item
1Physical Applicability of Self Gravitating Isothermal Sphere Equilibrium Theory III Dark Matter Galactic Halo Mass Densities Quantized Polytropic index, n(l), l a positive integer Galactic Rotation Curves James G. Gilson

Physical Applicability of Self Gravitating Isothermal Sphere Equilibrium Theory III Dark Matter Galactic Halo Mass Densities Quantized Polytropic index, n(l), l a positive integer Galactic Rotation Curves James G. Gilson

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Source URL: www.fine-structure-constant.org

Language: English - Date: 2012-12-16 13:05:55
2Dark Matter Detection: Finding a Halo in a Haystack Paul Covington, Dan Frank, Alex Ioannidis 1  Introduction

Dark Matter Detection: Finding a Halo in a Haystack Paul Covington, Dan Frank, Alex Ioannidis 1 Introduction

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Source URL: cs229.stanford.edu

Language: English - Date: 2013-01-09 20:22:36
    3Galaxy Formation Made Simple… thanks to Sloan! Sloan Science Symposium Sandra M . Faber August 1 5 ,

    Galaxy Formation Made Simple… thanks to Sloan! Sloan Science Symposium Sandra M . Faber August 1 5 ,

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    Source URL: sdss2008.uchicago.edu

    Language: English - Date: 2015-07-01 19:26:51
    4A novel approach to derive halo-independent limits on dark matter properties Sebastian Wild TUM, Munich

    A novel approach to derive halo-independent limits on dark matter properties Sebastian Wild TUM, Munich

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    Source URL: www.taup-conference.to.infn.it

    Language: English - Date: 2015-09-07 10:42:52
      5dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

      dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

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      Source URL: www.astro.rug.nl

      Language: English - Date: 2011-05-16 03:37:41
      6Ay 124 – Handouts 3 Asymmetric Drift and Star Streams Dehnen & Binney found that the V component (in the plane) of the sun’s motion depends on what kind of local

      Ay 124 – Handouts 3 Asymmetric Drift and Star Streams Dehnen & Binney found that the V component (in the plane) of the sun’s motion depends on what kind of local

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      Source URL: www.tapir.caltech.edu

      Language: English - Date: 2010-01-31 22:52:23
      7Ay 124 – Handout 5 Age-dating star clusters Isochrones can be used to predict the location (luminosity and color) of the main sequence turn-off and hence

      Ay 124 – Handout 5 Age-dating star clusters Isochrones can be used to predict the location (luminosity and color) of the main sequence turn-off and hence

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      Source URL: www.tapir.caltech.edu

      Language: English - Date: 2010-02-05 13:31:02
      8The Scalable Data Management, Analysis, and Visualization Institute http://sdav-scidac.org  Data Intensive Analysis Techniques and Tools M. M. A. Patwary (NWU), A. Agrawal (NWU), W. Liao (NWU), A. Choudhary (NWU), S. Hab

      The Scalable Data Management, Analysis, and Visualization Institute http://sdav-scidac.org Data Intensive Analysis Techniques and Tools M. M. A. Patwary (NWU), A. Agrawal (NWU), W. Liao (NWU), A. Choudhary (NWU), S. Hab

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      Source URL: sdav-scidac.org

      Language: English - Date: 2014-03-27 13:39:35
      9Introduction to simulation databases using CosmoSim Kristin Riebe∗, GAVO May 21, 2015

      Introduction to simulation databases using CosmoSim Kristin Riebe∗, GAVO May 21, 2015

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      Source URL: www.g-vo.org

      Language: English - Date: 2015-05-21 07:45:09
      10Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory – Paper Review Stephen Portillo Review of R. Abbasi et al. (IceCube Collaboration), Phys. Rev. D 84, ).

      Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory – Paper Review Stephen Portillo Review of R. Abbasi et al. (IceCube Collaboration), Phys. Rev. D 84, ).

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      Source URL: portillo.ca

      Language: English - Date: 2013-07-27 00:55:57