pith. sign in

Evanston)

Identifiers

  • name variant Evanston) 0.60 · backfill

Papers (5)

  1. How well do STARLAB and NBODY compare? II: Hardware and accuracy astro-ph.IM · 2012 · author #8
  2. Collisions Between Single Stars in Dense Clusters: Runaway Formation of a Massive Object astro-ph · 2004 · author #5
  3. Run-away formation of intermediate-mass black holes in dense star clusters astro-ph · 2004 · author #5
  4. Hadronic Decays of J/psi(1^{3}S_{1}) and psi'(2^{3}S_{1}) Through Vitrual Photons hep-ex · 2004 · author #2
  5. Spin effects in the inspiral of coalescing compact binaries gr-qc · 1992 · author #5

Mentions

  • 1201.5692 #8 · backfill · confidence 0.70 Evanston)

Frequent Coauthors