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相关论文: Hybrid morphology radio sources - follow-up VLBA o…

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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

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

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

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 (HyMoRS) are a class of radio galaxies having the lobe morphology of a Fanaroff-Riley (FR) type I on one side of the active nucleus and of a FR type II on the other. The origin of the different morphologies…

星系天体物理 · 物理学 2017-02-01 F. de Gasperin

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

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

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

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 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

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…

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

We present a new sample of 30 nearby (z<0.2) BL Lacs, selected to study the nuclear as well as the large scale properties of low power radio sources. In this first paper, we show and discuss new radio data taken with the VLA (19 objects at…

天体物理学 · 物理学 2009-11-10 M. Giroletti , G. Giovannini , G. B. Taylor , R. Falomo

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

We propose a morphological classification based on the parsec scale structure of fifty-one High Frequency Peakers (HFPs) from the ``bright'' HFP sample. VLBA images at two adjacent frequencies (chosen among 8.4, 15.3, 22.2 and 43.2 GHz)…

天体物理学 · 物理学 2009-11-11 M. Orienti , D. Dallacasa , S. Tinti , C. Stanghellini

VLBA observations are presented for 6 compact radio sources selected from the Peacock & Wall catalogue. From the new morphological and spectral information 2 objects that in the Peacock and Wall catalogue are flat spectrum (alpha < 0.5)…

天体物理学 · 物理学 2009-11-10 A. Rossetti , F. Mantovani , D. Dallacasa , C. Fanti , R. Fanti

We present sub-arcsecond ($\theta\sim0.1^{\prime\prime}$) resolution VLA 1.3 cm continuum and 22.2 GHz H$_2$O maser observations toward 15 compact radio continuum sources with rising spectral index and 8 string-like radio continuum…

太阳与恒星天体物理 · 物理学 2026-01-19 Tatiana M. Rodriguez , Peter Hofner , Emmanuel Momjian , Esteban D. Araya , Ananay Sethi , Viviana Rosero

Global VLBI observations at 5 GHz have been performed to study the source morphology in 10 compact steep-spectrum (CSS) sources selected from the Peacock & Wall catalogue with the aim of finding asymmetric structures produced by the…

宇宙学与河外天体物理 · 物理学 2015-06-15 D. Dallacasa , M. Orienti , C. Fanti , R. Fanti , C. Stanghellini

Extragalactic radio sources have been classified into two classes, Fanaroff-Riley I and II, which differ in morphology and radio power. Strongly emitting sources belong to the edge-brightened FR II class, and weakly emitting sources to the…

高能天体物理现象 · 物理学 2016-12-07 S. Massaglia , G. Bodo , P. Rossi , S. Capetti , A. Mignone
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