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相关论文: Multifrequency study of a double-double radio gala…

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We report the discovery of a double-double radio source (DDRS) J0028+0035. We observed it with LOFAR, GMRT, and the VLA. By combining our observational data with those from the literature, we gathered an appreciable set of radio flux…

星系天体物理 · 物理学 2020-12-29 A. Marecki , M. Jamrozy , J. Machalski , U. Pajdosz-Smierciak

We present radio continuum observations at frequencies ranging from $\sim$150 to 5000 MHz of the misaligned double-double radio galaxy, DDRG, 3C293 (J1352+3126) using the Giant Metrewave Radio Telescope (GMRT) and the Very Large Array…

宇宙学与河外天体物理 · 物理学 2015-05-27 S. A. Joshi , S. Nandi , D. J. Saikia , C. H. Ishwara-Chandra , C. Konar

We present new radio observations at frequencies ranging from 240 to 4860 MHz of the well-known, double-double radio galaxy (DDRG), J1453+3308, using both the Giant Metrewave Radio Telescope (GMRT) and the Very Large Array (VLA). These…

天体物理学 · 物理学 2009-11-11 C. Konar , D. J. Saikia , M. Jamrozy , J. Machalski

We present a multi-frequency analysis of the candidate double-double radio galaxy (DDRG) J2349-0003, exhibiting a possible lobe misalignment. High-resolution uGMRT observations at Bands 3 and 4 reveal a complex radio morphology featuring a…

星系天体物理 · 物理学 2025-07-15 Sudheesh T. P. , Ruta Kale , Jithesh V. , Ishwara-Chandra C. H. , Joe Jacob

We present a study of the peculiar radio galaxy B 1834+620. It is characterised by the presence of a 420-kpc large edge-brightened radio source which is situated within, and well aligned with, a larger (1.66 Mpc) radio source. Both sources…

天体物理学 · 物理学 2009-10-31 Arno P. Schoenmakers , A. G. de Bruyn , H. J. A. Rottgering , H. van der Laan

The excellent sensitivity and optimum resolution of LoTSS DR2 at 144 MHz has enabled us to discover a giant radio galaxy (J1225+4011) with three distinct episodes of jet activity, making it a member of a class of objects called…

星系天体物理 · 物理学 2023-08-02 Kshitij Chavan , Pratik Dabhade , D. J. Saikia

We present a radio and optical study of the double-double radio galaxy J1328+2752 based on new low-frequency GMRT observations and SDSS data. The radio data were used to investigate the morphology and to perform a spectral index analysis.…

星系天体物理 · 物理学 2017-04-19 S. Nandi , M. Jamrozy , R. Roy , J. Larsson , D. J. Saikia , M. Baes , M. Singh

Using the new low-frequency and high-frequency radio images of this galaxy, we determined the shape of the spectrum along its lobes and performed the classical spectral-ageing analysis. On the other hand, we applied the analytical model of…

宇宙学与河外天体物理 · 物理学 2015-05-14 J. Machalski , M. Jamrozy , C. Konar

We report the discovery of a grand-design spiral galaxy associated with a double-lobed radio source. J1649+2635 (z = 0.0545) is a red spiral galaxy with a prominent bulge that it is associated with a L$_{1.4{\rm…

We report the discovery of a double-double radio galaxy (DDRG), J0041+3224, with the Giant Metrewave Radio Telescope (GMRT) and subsequent high-frequency observations with the Very Large Array (VLA). The inner and outer doubles are aligned…

天体物理学 · 物理学 2009-11-13 D. J. Saikia , C. Konar , V. K. Kulkarni

We present radio observations at frequencies ranging from 240 to 8460 MHz of the radio galaxy 4C29.30 (J0840+2949) using the Giant Metrewave Radio Telescope (GMRT), the Very Large Array (VLA) and the Effelsberg telescope. We report the…

天体物理学 · 物理学 2008-11-26 M. Jamrozy , C. Konar , D. J. Saikia , L. Stawarz , K. -H. Mack , A. Siemiginowska

In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasars, which are still unclear, we have identified such sources with a large range of linear sizes (220 $-$ 917 kpc), and hence time scales of…

星系天体物理 · 物理学 2019-07-17 S. Nandi , D. J. Saikia , R. Roy , P. Dabhade , Y. Wadadekar , J. Larsson , M. Baes , H. C. Chandola , M. Singh

Double-double radio galaxies (DDRGs) offer a unique opportunity for us to study multiple episodes of jet activity in large-scale radio sources. We use radio data from the Very Large Array and the literature to model two DDRGs, B1450+333 and…

高能天体物理现象 · 物理学 2015-05-19 Catherine Brocksopp , Christian Kaiser , Arno Schoenmakers , Ger de Bruyn

The evolution of radio jet morphology and its energetics is significantly influenced by the environment in which the host galaxy resides. As giant radio galaxies (GRGs) often extend to the scale of entire galaxy clusters ($\sim$Mpc) and…

星系天体物理 · 物理学 2026-01-21 Shobha Kumari , Sabyasachi Pal , Surajit Paul , Marek Jamrozy

The existence of double-double radio galaxies (DDRGs) is evidence for recurrent jet activity in AGN, as expected from standard accretion models. A detailed study of these rare sources provides new perspectives for investigating the AGN duty…

We present ATCA radio observations of the giant radio galaxy J0116-473 at 12 and 22 cm wavelengths in total intensity and polarization. The images clearly reveal a bright inner-double structure within more extended edge-brightened lobe…

天体物理学 · 物理学 2009-11-07 Lakshmi Saripalli , Ravi Subrahmanyan , N. Udaya Shankar

Radio loud Active Galactic Nuclei are episodic in nature, cycling through periods of activity and quiescence. In this work we investigate the duty cycle of the radio galaxy B2~0258+35, which was previously suggested to be a restarted radio…

We report the discovery of an S-shaped morphology of the radio galaxy J0644$+$1043 imaged with a 30 $\mu$Jy sensitive 525 MHz broadband (band 3 $+$ 4) uGMRT map. Dedicated spectroscopic observations of the host galaxy carried out with the…

星系天体物理 · 物理学 2024-05-24 Sagar Sethi , Agnieszka Kuźmicz , Marek Jamrozy , Lyuba Slavcheva-Mihova

In this paper, we test the possibility that the structure of the largest radio galaxy J1420-0545 may have been formed by restarted rather than primary jet activity. This hypothesis was motivated by the unusual morphological properties of…

星系天体物理 · 物理学 2017-11-29 M. Jamrozy , J. Machalski , B. Nikiel-Wroczynski , H. T. Intema

Triple-double radio galaxies (TDRGs) are amongst the rarest subpopulations of radio galaxies (RGs). They are characterised by three pairs of radio lobes, where each pair of lobes represents an episode of nuclear activity. Such a feature…

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