37 GHz observations of narrow-line Seyfert 1 galaxiesLähteenmäki A.,
Järvelä E.,
Hovatta T.,
Tornikoski M.,
Harrison D.,
López-Caniego M.,
Max-Moerbeck W.,
Mingaliev M.,
Pearson T.,
Ramakrishnan V.,
Readhead A.,
Reeves R.,
Richards J.,
Sotnikova Y.,
Tammi J. . The spectra at a given time are often inverted or convex. The
source of the high-frequency
radio emission 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 сектореКозирацкий, Ю.Л.,
Паринов, М.Л.,
Мамаджанян, Е.А.,
Koziratsky, Yuriy L.,
Parinov, Maxim L.,
Mamadjanyan, Ervant А. The method correlation Measurement of coordinates the
radio emission sources, based on a