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Butyrivibrio sp. G52

 
National Institutes of Health

Papers overview

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2001
2001
Post-Newtonian smoothed particle hydrodynamics calculations of binary neutron star coalescence. II. Binary mass ratio, equation of state, and spin dependence
Using our new post-Newtonian SPH ~smoothed particle hydrodynamics! code, we study the final coalescence and merging of neutron… Expand
  • table I
  • table II
  • table III
  • figure 2
  • figure 1
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