On long-term variations of the total irradiance and on probable changes of temperature in the Sun's core

¹Abdussamatov HI. On long-term variations of the total irradiance and on probable changes of temperature in the Sun's core. 2005 ;21(6):471-477.

Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines

¹Stodilka MI. Diagnostics of the solar atmosphere by inverse methods: hydrogen absorption lines. 2005 ;21(6):461-470.

Spectral investigations of the symbiotic star CH Cygni

¹Mikailov KM, ¹Khalilov VM. Spectral investigations of the symbiotic star CH Cygni. 2005 ;21(6):452-460.

Close binary systems in regions of OB-Associations. III. V443 Cygni in Cyg OB9

¹Zakirov MM, ²Eshankulova MU. Close binary systems in regions of OB-Associations. III. V443 Cygni in Cyg OB9. 2005 ;21(6):441-451.

The structure of our stellar system

¹Zakhozhay VA. The structure of our stellar system. 2005 ;21(6):414-440.

A. Ya. Orlov and his astrogeodynamical scientific school

¹Yatskiv YS, Korsun' AA, ¹Vavilova IB. A. Ya. Orlov and his astrogeodynamical scientific school. 2005 ;21(6):403-413.

On application of a scanner for determination of coordinates and photometric characteristics of stars from the FON program plates

Andruk VN, ¹Ivanov GA, Pogorel'tsev MT, ¹Yatsenko AI. On application of a scanner for determination of coordinates and photometric characteristics of stars from the FON program plates. 2005 ;21(5):396-400.

Coupled finite element method for the Earth's orientation parameter problems

Lubkov MV. Coupled finite element method for the Earth's orientation parameter problems. 2005 ;21(5):389-395.

The study of gravitational fragmentation of colliding molecular clouds

Vinogradov SB, Berczik PP. The study of gravitational fragmentation of colliding molecular clouds. 2005 ;21(5):368-388.

On the sequence of the rise of plasma wave instabilities near the footpoints of solar arch structures at the early stages of a flare process

Kryshtal' AN, ¹Gerasimenko SV. On the sequence of the rise of plasma wave instabilities near the footpoints of solar arch structures at the early stages of a flare process. 2005 ;21(5):352-367.

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