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Sapienza

Identifiers

  • name variant Sapienza 0.60 · backfill

Papers (13)

  1. On the relation between the mass of Compact Massive Objects and their host galaxies astro-ph.GA · 2017 · author #3
  2. Globular cluster-massive black hole interactions in galactic centers astro-ph.GA · 2016 · author #2
  3. Decoding the stellar fossils of the dusty Milky Way progenitors astro-ph.GA · 2014 · author #6
  4. A Performance Comparison of Different Graphics Processing Units Running Direct N-Body Simulations astro-ph.IM · 2013 · author #3
  5. Dynamical Friction in Cuspidal Galaxies astro-ph.CO · 2013 · author #3
  6. The Dense Stellar Systems Around Galactic Massive Black Holes astro-ph.CO · 2013 · author #4
  7. Galactic Nuclear Cluster Formation Via Globular Cluster Mergers astro-ph.GA · 2013 · author #2
  8. A fully parallel, high precision, N-body code running on hybrid computing platforms astro-ph.IM · 2012 · author #4
  9. NBSymple, a double parallel, symplectic N-body code running on Graphic Processing Units astro-ph.IM · 2010 · author #4
  10. Simulations of Nuclear Cluster formation astro-ph.CO · 2009 · author #3
  11. Galactic Nuclei Formation Via Globular Cluster Merging astro-ph.GA · 2009 · author #3
  12. High performance computing for classic gravitational N-body systems astro-ph.IM · 2009 · author #2
  13. Merging of globular clusters within inner galactic regions. II. The Nuclear Star Cluster formation astro-ph · 2008 · author #3

Mentions

  • 1409.5798 #6 · backfill · confidence 0.70 Sapienza
  • 1304.1966 #3 · backfill · confidence 0.70 Sapienza
  • 1302.4088 #3 · backfill · confidence 0.70 Sapienza
  • 1302.2509 #4 · backfill · confidence 0.70 Sapienza
  • 1301.2899 #2 · backfill · confidence 0.70 Sapienza
  • 1207.2367 #4 · backfill · confidence 0.70 Sapienza
  • 1003.3896 #4 · backfill · confidence 0.70 Sapienza
  • 0902.0472 #3 · backfill · confidence 0.70 Sapienza
  • 0901.4932 #3 · backfill · confidence 0.70 Sapienza
  • 0901.1018 #2 · backfill · confidence 0.70 Sapienza
  • 0801.1072 #3 · backfill · confidence 0.70 Sapienza

Frequent Coauthors