Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array

Natasha Hurley-Walker; Melanie Johnston-Hollitt; Ron Ekers; Richard Hunstead; Elaine M. Sadler; Luke Hindson; Paul Hancock; Gianni Bernardi; Judd D. Bowman; Frank Briggs; Roger Cappallo; Brian Corey; Avinash A. Deshpande; David Emrich; Bryan M. Gaensler; Robert Goeke; Lincoln Greenhill; Bryna J. Hazelton; Jacqueline Hewitt; David L. Kaplan; Justin Kasper; Eric Kratzenberg; Colin Lonsdale; Mervyn Lynch; Daniel Mitchell; Russell McWhirter; Miguel Morales; Edward Morgan; Divya Oberoi; Andre Offringa; Stephen Ord; Thiagaraj Prabu; Alan Rogers; Anish Roshi; Udaya Shankar; K. Srivani; Ravi Subrahmanyan; Steven Tingay; Mark Waterson; Randall B. Wayth; Rachel Webster; Alan Whitney; Andrew Williams; Chris Williams

doi:10.1093/mnras/stu2570

Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array

Natasha Hurley-Walker, Melanie Johnston-Hollitt, Ron Ekers, Richard Hunstead, Elaine M. Sadler, Luke Hindson, Paul Hancock, Gianni Bernardi, Judd D. Bowman, Frank Briggs, Roger Cappallo, Brian Corey, Avinash A. Deshpande, David Emrich, Bryan M. Gaensler, Robert Goeke, Lincoln Greenhill, Bryna J. Hazelton, Jacqueline Hewitt, David L. KaplanJustin Kasper, Eric Kratzenberg, Colin Lonsdale, Mervyn Lynch, Daniel Mitchell, Russell McWhirter, Miguel Morales, Edward Morgan, Divya Oberoi, Andre Offringa, Stephen Ord, Thiagaraj Prabu, Alan Rogers, Anish Roshi, Udaya Shankar, K. Srivani, Ravi Subrahmanyan, Steven Tingay, Mark Waterson, Randall B. Wayth, Rachel Webster, Alan Whitney, Andrew Williams, Chris Williams

Research output: Contribution to journal › Article › peer-review

20 Citations (Scopus)

9 Downloads (Pure)

Abstract

Recent observations with the Murchison Widefield Array at 185~MHz have serendipitously unveiled a heretofore unknown giant and relatively nearby ($z = 0.0178$) radio galaxy associated with NGC\,1534. The diffuse emission presented here is the first indication that NGC\,1534 is one of a rare class of objects (along with NGC\,5128 and NGC\,612) in which a galaxy with a prominent dust lane hosts radio emission on scales of $\sim$700\,kpc. We present details of the radio emission along with a detailed comparison with other radio galaxies with disks. NGC1534 is the lowest surface brightness radio galaxy known with an estimated scaled 1.4-GHz surface brightness of just 0.2\,mJy\,arcmin$^{-2}$. The radio lobes have one of the steepest spectral indices yet observed: $\alpha=-2.1\pm0.1$, and the core to lobe luminosity ratio is $

Original language	English
Pages (from-to)	2468-2478
Number of pages	11
Journal	Monthly Notices of the Royal Astronomical Society
Volume	447
Issue number	3
DOIs	https://doi.org/10.1093/mnras/stu2570
Publication status	Published - 1 Mar 2015

Keywords

astro-ph.GA

Access to Document

10.1093/mnras/stu2570

Published VersionFinal published version, 5.09 MB

Cite this

Hurley-Walker, N., Johnston-Hollitt, M., Ekers, R., Hunstead, R., Sadler, E. M., Hindson, L., Hancock, P., Bernardi, G., Bowman, J. D., Briggs, F., Cappallo, R., Corey, B., Deshpande, A. A., Emrich, D., Gaensler, B. M., Goeke, R., Greenhill, L., Hazelton, B. J., Hewitt, J., ... Williams, C. (2015). Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array. Monthly Notices of the Royal Astronomical Society, 447(3), 2468-2478. https://doi.org/10.1093/mnras/stu2570

@article{a9a757766e62419397405f0e65850f44,

title = "Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array",

abstract = "Recent observations with the Murchison Widefield Array at 185~MHz have serendipitously unveiled a heretofore unknown giant and relatively nearby ($z = 0.0178$) radio galaxy associated with NGC\,1534. The diffuse emission presented here is the first indication that NGC\,1534 is one of a rare class of objects (along with NGC\,5128 and NGC\,612) in which a galaxy with a prominent dust lane hosts radio emission on scales of $\sim$700\,kpc. We present details of the radio emission along with a detailed comparison with other radio galaxies with disks. NGC1534 is the lowest surface brightness radio galaxy known with an estimated scaled 1.4-GHz surface brightness of just 0.2\,mJy\,arcmin$^{-2}$. The radio lobes have one of the steepest spectral indices yet observed: $\alpha=-2.1\pm0.1$, and the core to lobe luminosity ratio is $",

keywords = "astro-ph.GA",

author = "Natasha Hurley-Walker and Melanie Johnston-Hollitt and Ron Ekers and Richard Hunstead and Sadler, {Elaine M.} and Luke Hindson and Paul Hancock and Gianni Bernardi and Bowman, {Judd D.} and Frank Briggs and Roger Cappallo and Brian Corey and Deshpande, {Avinash A.} and David Emrich and Gaensler, {Bryan M.} and Robert Goeke and Lincoln Greenhill and Hazelton, {Bryna J.} and Jacqueline Hewitt and Kaplan, {David L.} and Justin Kasper and Eric Kratzenberg and Colin Lonsdale and Mervyn Lynch and Daniel Mitchell and Russell McWhirter and Miguel Morales and Edward Morgan and Divya Oberoi and Andre Offringa and Stephen Ord and Thiagaraj Prabu and Alan Rogers and Anish Roshi and Udaya Shankar and K. Srivani and Ravi Subrahmanyan and Steven Tingay and Mark Waterson and Wayth, {Randall B.} and Rachel Webster and Alan Whitney and Andrew Williams and Chris Williams",

note = "This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. {\textcopyright} 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.",

year = "2015",

month = mar,

day = "1",

doi = "10.1093/mnras/stu2570",

language = "English",

volume = "447",

pages = "2468--2478",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "1365-2966",

publisher = "Oxford University Press (OUP)",

number = "3",

}

Hurley-Walker, N, Johnston-Hollitt, M, Ekers, R, Hunstead, R, Sadler, EM, Hindson, L, Hancock, P, Bernardi, G, Bowman, JD, Briggs, F, Cappallo, R, Corey, B, Deshpande, AA, Emrich, D, Gaensler, BM, Goeke, R, Greenhill, L, Hazelton, BJ, Hewitt, J, Kaplan, DL, Kasper, J, Kratzenberg, E, Lonsdale, C, Lynch, M, Mitchell, D, McWhirter, R, Morales, M, Morgan, E, Oberoi, D, Offringa, A, Ord, S, Prabu, T, Rogers, A, Roshi, A, Shankar, U, Srivani, K, Subrahmanyan, R, Tingay, S, Waterson, M, Wayth, RB, Webster, R, Whitney, A, Williams, A & Williams, C 2015, 'Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array', Monthly Notices of the Royal Astronomical Society, vol. 447, no. 3, pp. 2468-2478. https://doi.org/10.1093/mnras/stu2570

TY - JOUR

T1 - Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array

AU - Hurley-Walker, Natasha

AU - Johnston-Hollitt, Melanie

AU - Ekers, Ron

AU - Hunstead, Richard

AU - Sadler, Elaine M.

AU - Hindson, Luke

AU - Hancock, Paul

AU - Bernardi, Gianni

AU - Bowman, Judd D.

AU - Briggs, Frank

AU - Cappallo, Roger

AU - Corey, Brian

AU - Deshpande, Avinash A.

AU - Emrich, David

AU - Gaensler, Bryan M.

AU - Goeke, Robert

AU - Greenhill, Lincoln

AU - Hazelton, Bryna J.

AU - Hewitt, Jacqueline

AU - Kaplan, David L.

AU - Kasper, Justin

AU - Kratzenberg, Eric

AU - Lonsdale, Colin

AU - Lynch, Mervyn

AU - Mitchell, Daniel

AU - McWhirter, Russell

AU - Morales, Miguel

AU - Morgan, Edward

AU - Oberoi, Divya

AU - Offringa, Andre

AU - Ord, Stephen

AU - Prabu, Thiagaraj

AU - Rogers, Alan

AU - Roshi, Anish

AU - Shankar, Udaya

AU - Srivani, K.

AU - Subrahmanyan, Ravi

AU - Tingay, Steven

AU - Waterson, Mark

AU - Wayth, Randall B.

AU - Webster, Rachel

AU - Whitney, Alan

AU - Williams, Andrew

AU - Williams, Chris

N1 - This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

PY - 2015/3/1

Y1 - 2015/3/1

N2 - Recent observations with the Murchison Widefield Array at 185~MHz have serendipitously unveiled a heretofore unknown giant and relatively nearby ($z = 0.0178$) radio galaxy associated with NGC\,1534. The diffuse emission presented here is the first indication that NGC\,1534 is one of a rare class of objects (along with NGC\,5128 and NGC\,612) in which a galaxy with a prominent dust lane hosts radio emission on scales of $\sim$700\,kpc. We present details of the radio emission along with a detailed comparison with other radio galaxies with disks. NGC1534 is the lowest surface brightness radio galaxy known with an estimated scaled 1.4-GHz surface brightness of just 0.2\,mJy\,arcmin$^{-2}$. The radio lobes have one of the steepest spectral indices yet observed: $\alpha=-2.1\pm0.1$, and the core to lobe luminosity ratio is $

AB - Recent observations with the Murchison Widefield Array at 185~MHz have serendipitously unveiled a heretofore unknown giant and relatively nearby ($z = 0.0178$) radio galaxy associated with NGC\,1534. The diffuse emission presented here is the first indication that NGC\,1534 is one of a rare class of objects (along with NGC\,5128 and NGC\,612) in which a galaxy with a prominent dust lane hosts radio emission on scales of $\sim$700\,kpc. We present details of the radio emission along with a detailed comparison with other radio galaxies with disks. NGC1534 is the lowest surface brightness radio galaxy known with an estimated scaled 1.4-GHz surface brightness of just 0.2\,mJy\,arcmin$^{-2}$. The radio lobes have one of the steepest spectral indices yet observed: $\alpha=-2.1\pm0.1$, and the core to lobe luminosity ratio is $

KW - astro-ph.GA

U2 - 10.1093/mnras/stu2570

DO - 10.1093/mnras/stu2570

M3 - Article

SN - 1365-2966

VL - 447

SP - 2468

EP - 2478

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array

Abstract

Keywords

Access to Document

Fingerprint

Cite this