Работы, цитирующие эту работу

Работ: 4

Работа: Lopsided Spiral Galaxies and a Limit on the Galaxy Accretion Rate

1. Gravitational instability of perturbations in a background nonlinear nonstationary model of a disk-like system. II. Large-scale tesseral oscillation modes

   K. T. Mirtadjieva

   СтатьяAstrophysics and Star Formation StudiesGravitation and Cosmology2012Цитирований: 6

   ABIABI:AkademIndex/openalex/2026.other.498485

2. Instabilities in a nonstationary model of self-gravitating disks. III. The phenomenon of lopsidedness and a comparison of perturbation modes

   K. T. Mirtadjieva, С. Н. Нуритдинов, J. K. Ruzibaev +1

   СтатьяAstro and Planetary ScienceAstrophysics2011Цитирований: 4

   ABIABI:AkademIndex/openalex/2011.article.000133

3. On the Theory of Formation of Lopsided Spiral Galaxies

   K. T. Mirtadjieva, С. Н. Нуритдинов, A. U. Omonov

   СтатьяGalaxies: Formation, Evolution, PhenomenaAstrophysical Bulletin2024Цитирований: 1

   ABIABI:AkademIndex/openalex/2024.article.003625

4. Analysis of data on lopsided galaxies and theories of their formation

   С. Н. Нуритдинов, K. T. Mirtadjieva, A. U. Omonov

   СтатьяGalaxies: Formation, Evolution, Phenomena2024Цитирований: 0

   ABIABI:AkademIndex/openalex/2024.article.009913