T. S. Konstantinova

1 ta ish

Institute of Applied Astronomy

1. THE STRUCTURE AND EMISSION MODEL OF THE RELATIVISTIC JET IN THE QUASAR 3C 279 INFERRED FROM RADIO TO HIGH-ENERGY γ-RAY OBSERVATIONS IN 2008-2010

   M. Hayashida, G. Madejski, Krzysztof Nalewajko +90

   MaqolaOAOchiq kirish20126 iqtibos

   ABIABI:AkademIndex/2026.other.058046