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相关论文: Blasting away a dwarf galaxy: The "tail" of ESO 32…

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From the LOFAR Two-metre Sky Survey second data release (LoTSS DR2) at 144 MHz, we identified a peculiar radio galaxy, J0011+3217. It has a large, one-sided diffuse secondary wing that stretches up to 0.85 Mpc (roughly 85\% of the size of…

星系天体物理 · 物理学 2024-09-25 Shobha Kumari , Sabyasachi Pal , Martin J. Hardcastle , Maya A. Horton

We present multi-frequency, radio-continuum and HI observations of NGC4438, the highly-disturbed, active galaxy in the Virgo cluster, with the VLA and the GMRT. High-resolution observations with the VLA at 4860 and 8460 MHz show the…

天体物理学 · 物理学 2009-11-13 Ananda Hota , D. J. Saikia , Judith A. Irwin

We report Australia Telescope Compact Array (ATCA) radio-continuum and ROSAT PSPC X-ray observations of the region surrounding the peculiar galaxy pair ESO 295-IG022, lying at the centre of the poor cluster Abell S0102. We identify a radio…

天体物理学 · 物理学 2009-11-06 A. M. Read , M. D. Filipovic , W. Pietsch , P. A. Jones

We report observations at mid-infrared and sub-millimeter wavelengths of Centaurus A (CenA, NGC 5128), the giant elliptical galaxy that harbors the closest radio loud Active Galactic Nucleus (AGN) to Earth. The dust emission from the deep…

We report new radio-continuum observations with the Australia Telescope Compact Array (ATCA) of the region surrounding the peculiar galaxy pair ESO 295-IG022, at the centre of the poor cluster Abell S0102. We observed this cluster at…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. D. Filipović , E. J. Crawford , P. A. Jones , G. L. White

We present measurements obtained with the Spitzer Space Telescope in five bands from 3.6-24 microns of the northern inner radio lobe of Centaurus A, the nearest powerful radio galaxy. We show that this emission is synchrotron in origin.…

天体物理学 · 物理学 2009-11-11 M. H. Brookes , C. R. Lawrence , J. Keene , D. Stern , V. Gorijan , M. Werner , V. Charmandaris

We present new radio and optical images of the nearest radio galaxy Centaurus A and its host galaxy NGC 5128. We focus our investigation on the northern transition region, where energy is transported from the ~5 kpc (~5 arcmin) scales of…

We present deep GALEX images of NGC 5128, the parent galaxy of Centaurus A. We detect a striking "weather ribbon" of Far-UV and H$\alpha$ emission, which extends more than 35 kpc northeast of the galaxy. The ribbon is associated with a…

星系天体物理 · 物理学 2015-06-23 Susan G. Neff , Jean A. Eilek , Frazer N. Owen

LOFAR observations at 144 MHz have revealed large-scale radio sources in the unrelaxed galaxy cluster Abell 1132. The cluster hosts diffuse radio emission on scales of $\sim$650 kpc near the cluster center and a head-tail (HT) radio galaxy,…

Here we re-analyze the archival {\it Chandra} data for the central parts of the Centaurus\,A radio galaxy, aiming for a systematic investigation of the X-ray emission associated with the inner radio lobes in the system, and their immediate…

高能天体物理现象 · 物理学 2020-11-10 Dominika Ł. Król , Volodymyr Marchenko , Michał Ostrowski , Łukasz Stawarz

This review summarizes the state of the knowledge of the nearby (D = 3.4 Mpc) radio source Centaurus A and its host galaxy NGC 5128. The massive elliptical host galaxy appears to be moderately triaxial. It contains a strongly warped thin…

天体物理学 · 物理学 2009-10-31 F. P. Israel

We present the results of an Australia Telescope Compact Array 1.4 GHz spectropolarimetric aperture synthesis survey of 34 square degrees centred on Centaurus A - NGC 5128. A catalogue of 1005 extragalactic compact radio sources in the…

NGC 5128 (Centaurus A) is one of the best targets to study AGN-feedback in the local Universe. Optical filaments located at 16 kpc from the galaxy along the radio jet direction show recent star formation, likely triggered by the interaction…

星系天体物理 · 物理学 2019-06-27 Quentin Salomé , Philippe Salomé , Antoine Gusdorf , Françoise Combes

We report on a spectral study at radio frequencies of the giant radio halo in A2142 (z=0.0909), which we performed to explore its nature and origin. A2142 is not a major merger and the presence of a giant radio halo is somewhat surprising.…

宇宙学与河外天体物理 · 物理学 2017-07-26 T. Venturi , M. Rossetti , G. Brunetti , D. Farnsworth , F. Gastaldello , S. Giacintucci , D. V. Lal , L. Rudnick , T. W. Shimwell , D. Eckert , S. Molendi , M. Owers

Centaurus A (Cen A) is the closest radio galaxy and a prime example of a low-luminosity active galactic nucleus (AGN), exhibiting complex emissions across the electromagnetic spectrum. The nature of its continuum emission, particularly the…

星系天体物理 · 物理学 2025-02-10 F. Marin , D. Hutsemékers , C. -Z. Jiang , R. Antonucci , P. M. Ogle , A. Bagul , C. Ramos Almeida , M. Berton

We present the results of new radio interferometer HI line observations for the merging galaxy pair NGC 4038/9 (`The Antennae'), obtained using the Australia Telescope Compact Array. The results improve substantially on those of van der…

天体物理学 · 物理学 2009-11-06 S. Gordon , B. Koribalski , K. Jones

Among the bent tail radio galaxies common in galaxy clusters are some with long, collimated tails (so-called head-tail galaxies) shaped by their interactions with the intracluster medium (ICM). Here we report the discovery of intricate…

ESO422-G028 denotes the very center cD-galaxy of the giant radio source B0503-286 (Saripalli et al. 1986, Subrahmanya and Hunstead, 1986). The angular extent of the associated radio structure is about 42.4 arcmin, which corresponds to a…

天体物理学 · 物理学 2007-05-23 M. Jamrozy , J. Kerp , U. Klein , K. -H. Mack , L. Saripalli

We present new radio continuum observations of two dwarf starburst galaxies, NGC3125 and NGC5408, with observations at 4.80GHz (6cm) and 8.64GHz (3cm), taken with the Australia Telescope Compact Array (ATCA). Both galaxies show a complex…

天体物理学 · 物理学 2009-11-07 Ian R. Stevens , Duncan A. Forbes , Ray P. Norris

We identify optical emission-line features 700" (12 kpc) southwest of the nucleus of Centaurus A, roughly opposite the radio jet and well-known optical emission filaments associated with the northern radio structure. These regions are…

星系天体物理 · 物理学 2019-01-30 William C. Keel , Julie K. Banfield , Anne Medling , Susan G. Neff
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