Science, Volume 319, Issues 5859-5864John Michels (Journalist) American Association for the Advancement of Science, 2008 |
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Page 50
... dark matter . The search for these lumps , lit up by stars that formed within them , is a major astronomical endeavor , although it has failed to find the huge expected population . Is this a dark matter crisis , or does it provide ...
... dark matter . The search for these lumps , lit up by stars that formed within them , is a major astronomical endeavor , although it has failed to find the huge expected population . Is this a dark matter crisis , or does it provide ...
Page 175
... dark matter and 370 Mo for gas . The mass of particles gen- erated to represent stars was 120 Mo. At the end of the simulations , the total numbers of dark- matter , gas , and star particles were 1.1 × 107 , 4.5 × 106 , and 4.5 × 105 ...
... dark matter and 370 Mo for gas . The mass of particles gen- erated to represent stars was 120 Mo. At the end of the simulations , the total numbers of dark- matter , gas , and star particles were 1.1 × 107 , 4.5 × 106 , and 4.5 × 105 ...
Page 176
... dark - matter - only simulations . -3 Whereas the dwarf galaxy halo in the dark- matter - only simulation develops a central cusp with logarithmic slope -0.95 , which is con- sistent with previous predictions of the standard model ( 7 ) ...
... dark - matter - only simulations . -3 Whereas the dwarf galaxy halo in the dark- matter - only simulation develops a central cusp with logarithmic slope -0.95 , which is con- sistent with previous predictions of the standard model ( 7 ) ...
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