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37 GHz observations of narrow-line Seyfert 1 galaxies. The spectra at a given time are often inverted or convex. The source of the high-frequency radio emission

Построение поверхности уровня радиоизлученияCreation of radio emission level

X-ray emission from accretion disks in active galactic nuclei and their X-ray emission cannot be explained by this model. © 2002 MAIK "Nauka/Interperiodica".

SRG/eROSITA uncovers the most X-ray luminous quasar at z > 6+544717 is its X-ray brightness relative to the optical/UV emission. We argue that it may be linked to its radio

An observational argument against accretion in magnetars, the persistent emission of anomalous X-ray pulsars (AXPs) is powered by the decay of the magnetic field. However

ATMOSPHERIC DISPERSION OF HYDROCARBON EMISSIONS FROM MOTOR FUEL STORAGE FACILITIES, the pollution of atmospheric air by hydrocarbon emissions at the local level on the example of the city

Корреляционный метод поиска и координатометрии излучающего радиоэлектронного средства в заданном сектореThe method correlation Measurement of coordinates the radio emission sources, based on a

The comparative accuracy of photographic observations of radio stars observed at the Engelhardt Astronomical Observatory Galactic Radio Sources (GRS) in the system PPM catalogue (Rizvanov & Dautov 1998). Analysis

Search for Candidate Objects with the Sunyaev–Zeldovich Effect in the Radio Source Vicinities—galaxies: clusters: general
with removed low multipoles in the direction to radio sources.

ОЦЕНКА ТОЧНОСТИ ОПРЕДЕЛЕНИЯ МЕСТОПОЛОЖЕНИЯ ИСТОЧНИКА РАДИОИЗЛУЧЕНИЯ С ПОМОЩЬЮ ЛЧМ ИОНОЗОНДА-РАДИОПЕЛЕНГАТОРАThe results of a single-position determination of the location of radio emission source (RES

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