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Иш: Nonlinear cosmogony of the spiral galaxy bulges

Instabilities in a nonstationary model of self-gravitating disks. I. Bar and ring perturbation modes
С. Н. Нуритдинов, K. T. Mirtadjieva, Mariam Sultana
МақолаAstrophysics and Star Formation StudiesAstrophysics200814 иқтибос
ABI
Instabilities in a nonstationary model of self-gravitating disks. II. Warp modes of vertical oscillations
С. Н. Нуритдинов, K. T. Mirtadjieva, Iqbal Ahmad +1
МақолаAstrophysics and Star Formation StudiesAstrophysics20097 иқтибос
ABI
Physics of Gravitating Systems I
A. M. Fridman, V. L. Polyachenko
Китоб19847 иқтибос
ABI
Dynamics of the Bending of the Galaxy
C. Hunter, Alar Toomre
Мақола19697 иқтибос
ABI
Models of clusters of point masses with quadratic gravitational potential
Г. С. Бисноватый-Коган, Ya. B. Zel’dovich
Мақола19705 иқтибос
ABI
Gravitational instability of perturbations in a background nonlinear nonstationary model of a disklike system. III. Large-scale bending oscillations modes
K. T. Mirtadjieva
МақолаAstrophysics and Star Formation StudiesGravitation and Cosmology20125 иқтибос
ABI
Bulges and ellipticals: can formation mechanisms be the same?
С. Н. Нуритдинов
Мақола19934 иқтибос
ABI
The globular cluster system of the galaxy. IV - The halo and disk subsystems
R. Zinn
Мақола19852 иқтибос
ABI
Evidence from the motions of old stars that the Galaxy collapsed.
O. J. Eggen, D. Lynden–Bell, Allan Sandage
Мақола19622 иқтибос
ABI
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