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Related papers: The remnant radio galaxy associated with NGC 1534

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(abridged) NGC 1569 is a nearby dwarf irregular galaxy which underwent an intense burst of star formation 10 to 40 Myr ago. We present observations that reach surface brightnesses two to eighty times fainter than previous radio continuum…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Amanda A. Kepley , Stefanie Muehle , John Everett , Ellen G. Zweibel , Eric M. Wilcots , Uli Klein

We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7 GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 sources (71 per cent) are unresolved in the new observations…

Astrophysics of Galaxies · Physics 2020-02-19 I. H. Whittam , D. A. Green , M. J. Jarvis , J. M. Riley

Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal…

Astrophysics · Physics 2009-11-06 Varoujan Gorjian , Jean L. Turner , Sara C. Beck

The Andromeda galaxy is the best-known large galaxy besides our own Milky Way. Several images and studies exist at all wavelengths from radio to hard X-ray. Nevertheless, only a few observations are available in the microwave range where…

We have used the Very Large Array aperture synthesis telescope to conduct a radio continuum survey of polar-ring galaxies, at 20cm and 6cm. Forty objects were observed at 20cm with 5" resolution. Twenty (50%) of the program sources were…

Astrophysics · Physics 2009-11-10 A. L. Cox , L. S. Sparke

Coherent low-frequency ($\lesssim 200$ MHz) radio emission from stars encodes the conditions of the outer corona, mass-ejection events, and space weather. Previous low-frequency searches for radio emitting stellar systems have lacked the…

It is now established that the faint radio population is a mixture of star-forming galaxies and faint active galactic nuclei (AGNs), with the former dominating below S(1.4GHz) \sim 100 muJy and the latter at larger flux densities. The faint…

Astrophysics of Galaxies · Physics 2018-12-26 R. Ricci , I. Prandoni , H. R. De Ruiter , P. Parma

We present radio observations at 1.5 GHz of 32 local objects selected to reproduce the physical properties of $z\sim5$ star-forming galaxies. We also report non-detections of five such sources in the sub-millimetre. We find a radio-derived…

Astrophysics of Galaxies · Physics 2017-06-28 Stephanie M. L. Greis , Elizabeth R. Stanway , Andrew J. Levan , Luke J. M. Davies , J. J. Eldridge

Low frequency observations at 325 and 610 MHz have been carried out for two "radio-loud" Seyfert galaxies, NGC4235 and NGC4594 (Sombrero galaxy), using the Giant Meterwave Radio Telescope (GMRT). The 610 MHz total intensity and 325-610 MHz…

Astrophysics of Galaxies · Physics 2016-04-20 P. Kharb , S. Srivastava , V. Singh , J. F. Gallimore , C. H. Ishwara-Chandra , Ananda Hota

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 S. A. Joshi , S. Nandi , D. J. Saikia , C. H. Ishwara-Chandra , C. Konar

New radio continuum (8 GHz and 1.4 GHz) and HI 21 cm line observations of the Seyfert 2 galaxy IC 5063 (PKS 2048-572) were obtained with the Australia Telescope Compact Array (ATCA). The 8 GHz image reveals a linear triple structure (~4'',…

Astrophysics · Physics 2009-10-30 R. Morganti , T. Oosterloo , Z. Tsvetanov

We present the results of a detailed analysis of the newly discovered 15 arcmin large FRII-type radio galaxy WNB 0313+683. It has a redshift of 0.0901 +/- 0.0002 and a projected linear size of 2.0 Mpc. Using multi-frequency radio data from…

We present the results of new radio observations carried out with the Karl G. Jansky Very Large Array C-configuration at 5.5 GHz for a sample of southern narrow-line Seyfert 1 galaxies (NLS1s). This work increases the number of known…

Astrophysics of Galaxies · Physics 2020-09-02 S. Chen , E. Jarvela , L. Crepaldi , M. Zhou , S. Ciroi , M. Berton , P. Kharb , L. Foschini , M. Gu , G. La Mura , A. Vietri

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…

Astrophysics · Physics 2008-11-26 M. Jamrozy , C. Konar , D. J. Saikia , L. Stawarz , K. -H. Mack , A. Siemiginowska

We present a multi-wavelength study of IC 1531 (z=0.02564), an extragalactic radio source associated with the $\gamma$-ray object 3FGL J0009.9-3206 and classified as a blazar of uncertain type in the Third Fermi Large Area Telescope AGN…

High Energy Astrophysical Phenomena · Physics 2018-10-17 T. Bassi , G. Migliori , P. Grandi , C. Vignali , M. A. Pérez-Torres , R. D. Baldi , E. Torresi , A. Siemiginowska , C. Stanghellini

G315.4-2.3 is an extended shell supernova remnant (SNR) with some characteristics of evolutionarily young remnants and some of older ones. To further elucidate some of its characteristics, we present imaging and polarimetry of this SNR at a…

Astrophysics · Physics 2009-10-31 John R. dickel , Richard G. Strom , D. K. Milne

The nearby dwarf starburst galaxy NGC5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded by thermal radio emission (the `radio nebula'). To investigate the role of these…

We present a new catalogue of radio sources in the face-on spiral galaxy M83. Radio observations taken in 2011, 2015, and 2017 with the Australia Telescope Compact Array (ATCA) at 5.5 and 9 GHz have detected 270 radio sources. Although a…

Astrophysics of Galaxies · Physics 2020-05-13 Thomas D. Russell , Richard L. White , Knox S. Long , William P. Blair , Roberto Soria , P. Frank Winkler

We present the serendipitous discovery of 8 distant ($>$ 50 pc) late M dwarfs with plausible associated radio emission at 144 MHz. The M dwarf nature of our sources has been confirmed with optical spectroscopy performed using HET/LRS2 and…

The results of multi-epoch observations of the southern starburst galaxy, NGC 253, with the Australian Long Baseline Array (LBA) at 2.3 GHz are presented. As with previous radio interferometric observations of this galaxy, no new sources…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Hayden Rampadarath , John S. Morgan , Emil Lenc , Steven J. Tingay