Dragoljub Marković

1 ta ish

University of Illinois Urbana-Champaign

1. Properties of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>r</mml:mi></mml:math>modes in rotating magnetic neutron stars. I. Kinematic secular effects and magnetic evolution equations

   Luciano Rezzolla, Frederick K. Lamb, Dragoljub Marković +1

   MaqolaOAOchiq kirish20015 iqtibos

   ABIABI:AkademIndex/2026.other.013381