Россия
Россия
Россия
Россия
УДК 520 Инструменты, приборы и методы астрономических наблюдений, измерений и анализа
УДК 520.2 Телескопы
УДК 524.82 Наблюдательная космология
УДК 524.74 Типы галактик
УДК 524.7-7 Характер излучения
ГРНТИ 41.29 Космология
ГРНТИ 41.27 Звездные системы
ГРНТИ 41.17 Астрофизика
ГРНТИ 41.51 Обсерватории. Инструменты, приборы и методы астрономических наблюдений
ОКСО 03.05.01 Астрономия
ББК 223 Физика
ТБК 6143 Астрофизика. Радиоастрономия
ТБК 6146 Космогония. Космология
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
The Big Trio program, based on steep and ultra-steep spectrum sources from RATAN-600 Cold Experiment surveys, targeted distant radio galaxies. New multiwavelength surveys enabled indepth analysis of 113 sources to determine their evolutionary status, environmental characteristics, and long-term spectral changes. Analysis revealed that 20% show signs of initial, fading, or resumed activity. Twenty four sources reside in galaxy groups/clusters or show jet reorientation; four paired sources have parent galaxies just tens of kpc apart. Spectral index analysis ($\alpha \leq -0.9$) showed a declining trend: 90 sources (out of 113) met the criterion in the 365-3940 MHz range (pre-1996 data), dropping to 70 in 340-3000 MHz (modern surveys) and 39 in 76-226 MHz (GLEAM). This decrease stems from instrumental effects (angular resolution differences affecting flux density measurements) and improved low-frequency spectral characterization. For individual sources, spectral index variations may also reflect intrinsic evolutionary processes and source variability.
active galaxies: high-redshift radio galaxies; general radio continuum
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