J1649+2635: A Grand-Design Spiral with a Large Double-Lobed Radio Source
arXiv:1410.8520 · doi:10.1093/mnras/stu2302
Abstract
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 L10WHz double-lobed radio source that spans almost 100kpc. J1649+2635 has a black hole mass of M 3--7 10M and SFR 0.26 -- 2.6Myear. The galaxy hosts a 96kpc diffuse optical halo, which is unprecedented for spiral galaxies. We find that J1649+2635 resides in an overdense environment with a mass of MM, likely a galaxy group below the detection threshold of the ROSAT All-Sky Survey. We suggest one possible scenario for the association of double-lobed radio emission from J1649+2635 is that the source may be similar to a Seyfert galaxy, located in a denser-than-normal environment. The study of spiral galaxies that host large-scale radio emission is important because although rare in the local Universe, these sources may be more common at high-redshifts.
arXiv comment11 pages, 9 figures, Accepted for publication in MNRAS
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