Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: Towards the ultimate conservative difference scheme. IV. A new approach to numerical convection

1. Rotating stars in relativity

   Vasileios Paschalidis, Nikolaos Stergioulas

   МақолаPulsars and Gravitational Waves ResearchLiving Reviews in Relativity20172 иқтибос

   ABIABI:AkademIndex/openalex/2017.article.000003

2. Moving Node Method for Differential Equations

   Umurdin Dalabaev, Malika Ikramova

   БобDifferential Equations and Numerical MethodsIntechOpen eBooks20231 иқтибос

   ABIABI:AkademIndex/openalex/2023.chapter.000138

3. Mass loss evolution and the formation of detached shells around TP-AGB stars

   Lars Mattsson, S. Höfner, Falk Herwig

   МақолаStellar, planetary, and galactic studiesAstronomy and Astrophysics20070 иқтибос

   ABIABI:AkademIndex/openalex/2007.article.000027