Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range

According to the long-term monitoring on 3 radio band frequencies (4.8, 8 and 14.5 GHz) obtained at the Observatory of the University of Michigan, studied extragalactic radio sources 3C 120, CTA 102, DA 55, and OJ 287. According to apply Fourier methods and wavelet analysis, which revealed a change...

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Main Authors: A. L. Suharev, M. I. Ryabov, A. I. Donskix, M. Aller
Format: Article
Language:English
Published: National Aviation University 2013-10-01
Series:Вісник Астрономічної школи
Subjects:
Online Access:http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/Suharev_et_al.html
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author A. L. Suharev
M. I. Ryabov
A. I. Donskix
M. Aller
author_facet A. L. Suharev
M. I. Ryabov
A. I. Donskix
M. Aller
author_sort A. L. Suharev
collection DOAJ
description According to the long-term monitoring on 3 radio band frequencies (4.8, 8 and 14.5 GHz) obtained at the Observatory of the University of Michigan, studied extragalactic radio sources 3C 120, CTA 102, DA 55, and OJ 287. According to apply Fourier methods and wavelet analysis, which revealed a change of harmonic signal components over time. Identified long-period (trend) and short-period components for each source at all frequencies studied. According to the VLBI studied the movement of bright component in the jet.
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spelling doaj.art-f3bc736eb2684e43a173e6a0816c0a452022-12-21T18:19:15ZengNational Aviation UniversityВісник Астрономічної школи1607-28552411-66022013-10-0191859210.18372/2411-6602.09.10852411-6602.09.1085Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave rangeA. L. Suharev0M. I. Ryabov1A. I. Donskix2M. Aller3Odessa Observatory, Institute of Radio Astronomy, NAS of UkraineOdessa Observatory, Institute of Radio Astronomy, NAS of UkraineOdessa National University, UkraineRadio Astronomy Observatory, University of Michigan, USAAccording to the long-term monitoring on 3 radio band frequencies (4.8, 8 and 14.5 GHz) obtained at the Observatory of the University of Michigan, studied extragalactic radio sources 3C 120, CTA 102, DA 55, and OJ 287. According to apply Fourier methods and wavelet analysis, which revealed a change of harmonic signal components over time. Identified long-period (trend) and short-period components for each source at all frequencies studied. According to the VLBI studied the movement of bright component in the jet.http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/Suharev_et_al.htmlextragalactic radio sourcesphysical properties
spellingShingle A. L. Suharev
M. I. Ryabov
A. I. Donskix
M. Aller
Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
Вісник Астрономічної школи
extragalactic radio sources
physical properties
title Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
title_full Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
title_fullStr Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
title_full_unstemmed Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
title_short Variability flux of extragalactic sources DА55, CTA 102, 3C 120 AND OJ 287 in microwave range
title_sort variability flux of extragalactic sources dа55 cta 102 3c 120 and oj 287 in microwave range
topic extragalactic radio sources
physical properties
url http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/Suharev_et_al.html
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