pith. sign in

Fr.)

Identifiers

  • name variant Fr.) 0.60 · backfill

Papers (3)

  1. Viscous dissipation by tidally forced inertial modes in a rotating spherical shell astro-ph.SR · 2009 · author #2
  2. Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds X. CO emission from star formation regions in LMC and SMC astro-ph · 2003 · author #20
  3. Can high energy cosmic rays be vortons ? hep-ph · 1997 · author #4

Mentions

  • 0909.3922 #2 · backfill · confidence 0.70 Fr.)

Frequent Coauthors