M. M. Romanova

1 ta ish

Cornell University

1. Magnetohydrodynamic Simulations of Disk–Magnetized Star Interactions in the Quiescent Regime: Funnel Flows and Angular Momentum Transport

   M. M. Romanova, G. V. Ustyugova, A. V. Koldoba +1

   MaqolaOAOchiq kirish20024 iqtibos

   ABIABI:AkademIndex/2026.other.009788