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 (MNRAS) |
| Volume | 447 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - 1 Mar 2015 |
Keywords
- astro-ph.GA
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