2003
DOI: 10.1023/a:1025453730995
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Cited by 7 publications
(8 citation statements)
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References 7 publications
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“…Adding the two distributions yields the observed distribution function for these objects. It should be noted that we predicted the existence of two subtypes of FRI extragalactic radio sources before (Andreasyan, 2012). As stated in the Introduction, we have proposed (Andreasyan & Sol (1999), Andreasyan & Sol (2000); Andreasyan et al (2002)) a mechanism for the formation of extragalactic radio sources involving features of the dynamics of clouds of relativistic electrons with different densities ejected from the central region of the parent galaxy in the assumed dipole magnetic field of the galaxy.…”
Section: Distribution Of the Elongation Parameter Of The Extragalactic Radio Sources For The Different Fr Classesmentioning
confidence: 53%
See 1 more Smart Citation
“…Adding the two distributions yields the observed distribution function for these objects. It should be noted that we predicted the existence of two subtypes of FRI extragalactic radio sources before (Andreasyan, 2012). As stated in the Introduction, we have proposed (Andreasyan & Sol (1999), Andreasyan & Sol (2000); Andreasyan et al (2002)) a mechanism for the formation of extragalactic radio sources involving features of the dynamics of clouds of relativistic electrons with different densities ejected from the central region of the parent galaxy in the assumed dipole magnetic field of the galaxy.…”
Section: Distribution Of the Elongation Parameter Of The Extragalactic Radio Sources For The Different Fr Classesmentioning
confidence: 53%
“…Here we bring some results (physical and morphological differences in different classes of extragalactic radio sources) obtained in our early study (Andreasyan & Sol (1999); Andreasyan & Sol (2000); Andreasyan et al (2002); Andreasyan et al (2013)) as well as some new results. The samples 1 and 2 with the references can be found in Andreasyan (2012), while sample 3 is in Andreasyan et al (2013) 5. The correlation of radio axis with the optical axis in nearby radio galaxies Data from sample of 267 nearby radio galaxies were used to study the correlations of radio axes with the optical axes of parent galaxies.…”
Section: Observational Datamentioning
confidence: 99%
“…In the calculations this condition was met for most of the region of the galaxy that was studied. An analogous procedure has already been used [6] for a detailed study of the magnetic field in the direction of the spiral arm of Sagittarius.…”
Section: Dm(r) As a Function Of Distance R It Is Evident From Eq (1mentioning
confidence: 99%
“…In particular, the pulsar distances are used together with Faraday rotation data to study the magnetic field of the galaxy. It should be pointed out that in a study of the magnetic fields in those directions where the pulsars are still in a given spiral arm even for distance variations over quite wide limits [6], the uncertainty in the distances of the pulsars is not important. However, some recent papers [7][8][9] contain studies of the fine structures of the magnetic fields in the inner spiral arms of the galaxy.…”
Section: Introductionmentioning
confidence: 99%
“…Kuzeyde Tokat güneyde Halep, gezgin ve tacirlerin kesişme noktalarıydı ve Doğuya kıvrılan yolların en önemlileri bu iki şehir üzerinden Musul'a geçmekteydi; Simeon, Tavernier ve Tournefort Tokat'ın Doğu'nun ''en mühim'' kesişme noktalarından ve ''Küçük Asya'nın ticaret merkezi'' olduğunu kaydetmiştir 92. Aynı zamanda Tokat ordu için, Bağdat'a uzanan askerî bir güzergâhtı 93. Bir kervan için Musul-Tokat arası bir ay sürmekte, Musul'dan gelen kervanın Tokat'a bez, boyalı tülbent ve palamut taşıdığı, önceleri Hintli ve İranlı tacirlerin Musul üzerinden Tokat'a gittikleri, ancak bunun uzun zaman kesintiye uğradığı belirtilmiştir 94.…”
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