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相关论文: Multifrequency study of a new Hybrid Morphology Ra…

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Hybrid morphology radio sources (HyMoRS) are a rare group of radio galaxies in which differing Fanaroff & Riley morphologies (FR I/II) are observed for each of the two lobes. While they potentially provide insights into the formation of…

星系天体物理 · 物理学 2019-11-11 Jeremy J. Harwood , Tessa Vernstrom , Andra Stroe

The so-called HYbrid MOrphology Radio Sources (HYMORS) are a class of objects that appear to have a mixed Fanaroff-Riley (FR) morphology in a single object; i.e. a HYMORS has an FR I-type lobe on one side of its nucleus and an FR II-type…

天体物理学 · 物理学 2009-11-13 M. P. Gawronski , A. Marecki , M. Kunert-Bajraszewska , A. J. Kus

A small subset of extragalactic double radio sources, termed HYMORS (HYbrid MOrpholgy Radio Sources), is distinguished by a very unusual, hybrid morphology in terms of the Fanaroff-Riley (FR) classification. In HYMORS, one radio lobe…

星系天体物理 · 物理学 2023-02-22 Gopal-Krishna , Paul J. Wiita , Ravi Joshi , Dusmanta Patra

Based on their differing radio morphologies, powerful radio galaxies can be separated into the Fanaroff-Riley I (FR-I) and II (FR-II) classes. Hybrid morphology radio sources (HyMoRS) contain morphologies consistent with each type of jet on…

星系天体物理 · 物理学 2022-12-28 Andra Stroe , Victoria Catlett , Jeremy J. Harwood , Tessa Vernstrom , Beatriz Mingo

Hybrid Morphology Radio Sources (HyMoRS) are a very rare subclass of radio galaxies with apparent mixed FR morphology, i.e. these galaxies seem to have an FR-I structure on one side of the core and an FR-II structure on the other side of…

星系天体物理 · 物理学 2022-09-05 Shobha Kumari , Sabyasachi Pal

Hybrid morphology radio sources (HyMoRSs) are a rare subclass of radio galaxies that display a Fanaroff-Riley type I (FR I) morphology on one side of the central supermassive black hole (SMBH) and a type II (FR II) morphology on the other.…

星系天体物理 · 物理学 2025-11-04 Souvik Manik , Shobha Kumari , Netai Bhukta , Sabyasachi Pal , Sushanta K. Mondal

We provide observational and theoretical perspectives on the currently much debated issue of the Fanaroff-Riley (FR) morphological dichotomy of extragalactic radio sources. In this context we introduce a new, albeit rare, class of double…

天体物理学 · 物理学 2007-05-23 Gopal-Krishna , Paul J. Wiita

The FRI/FRII dichotomy is a much debated issue in the astrophysics of extragalactic radio sources. Study of the properties of HYbrid MOrphology Radio Sources (HYMORS) may bring crucial information and lead to a step forward in understanding…

宇宙学与河外天体物理 · 物理学 2015-06-16 Maciej Ceglowski , Marcin Gawronski , Magdalena Kunert-Bajraszewska

A small fraction of double radio sources show a peculiar and striking hybrid morphology; they have a distinctly FR I structure on one side of the nucleus, and a FR II structure on the other. We argue that the mere existence of these HYMORS…

天体物理学 · 物理学 2007-05-23 Gopal-Krishna , Paul J. Wiita

Hybrid morphology radio sources are a rare type of radio galaxy that display different Fanaroff-Riley classes on opposite sides of their nuclei. To enhance the statistical analysis of hybrid morphology radio sources, we embarked on a…

Hybrid sources that present FR I - like jet on the one side of the radio core and FR II - like on the other are rare class of objects that may posses key to understanding the origin of FR division. We presents information connected with the…

星系天体物理 · 物理学 2015-04-03 Maciej Ceglowski , Marcin Gawronski , Magdalena Kunert-Bajraszewska

The advent of next-generation telescope facilities brings with it an unprecedented amount of data, and the demand for effective tools to process and classify this information has become increasingly important. This work proposes a novel…

We present here the polarization image of the hybrid morphology (HYMOR) and broad-absorption line (BAL) quasar PG1004+130 at 694~MHz obtained with the upgraded Giant Metrewave Radio Telescope (uGMRT). We detect linear polarization in this…

星系天体物理 · 物理学 2023-09-15 Salmoli Ghosh , P. Kharb , J. Baghel , S. Silpa

Powerful radio galaxies exist as either compact or extended sources, with the extended sources traditionally classified by their radio morphologies as Fanaroff--Riley (FR) type I and II sources. FRI/II and compact radio galaxies have also…

星系天体物理 · 物理学 2017-04-26 H. Miraghaei , P. N. Best

We present Chandra observations of the hybrid morphology radio sources 3C 433 and 4C 65.15, two members of the rare class of objects possessing an FR I jet on one side of the core and an FR II lobe on the other. The X-ray spectrum of 3C 433…

星系天体物理 · 物理学 2011-02-11 B. P. Miller , W. N. Brandt

X-shaped radio galaxies are defined by their peculiar large-scale radio morphology. In addition to the classical double-lobed structure they have a pair of low-luminosity wings that straddles the nucleus at almost right angles to the active…

宇宙学与河外天体物理 · 物理学 2015-05-19 Hermine Landt , Chi C. Cheung , Stephen E. Healey

Extragalactic radio sources appear under different morphologies, the most frequent ones are classified as Fanaroff-Riley type I (FR I), typically with lower luminosities, and Fanaroff-Riley type II, (FR II), typically more luminous. This…

高能天体物理现象 · 物理学 2022-03-23 S. Massaglia , G. Bodo , P. Rossi , A. Capetti , A. Mignone

Results from Chandra-HST-VLA observations of 13 hybrid sources are presented. Data from ten sources in the literature are analysed along with new data from three hybrid blazars belonging to the MOJAVE sample. Studies of such hybrid sources…

星系天体物理 · 物理学 2015-06-23 Preeti Kharb , Ethan Stanley , Matthew Lister , Herman Marshall , Chris O'Dea , Stefi Baum

Extended extragalactic radio sources have traditionally been classified into FR I and II types, based on the ratio r of the separation S between the brightest regions on either sides of the host galaxy and the total size T of the radio…

宇宙学与河外天体物理 · 物理学 2015-05-19 Yen-Ting Lin , Yue Shen , Michael Strauss , Gordon Richards , Ragnhild Lunnan

We examine relationships between the morphology in double radio sources and the radio-optical position angle offset--the relative orientation of the radio axis with respect to the major axis of the host galaxy. The study was done for a…

天体物理学 · 物理学 2011-02-11 Lakshmi Saripalli , Ravi Subrahmanyan
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