Spectacular 240 kpc double-sided relativistic jets in a spiral-hosted narrow-line Seyfert 1 galaxy
A. Vietri, E. J\"arvel\"a, M. Berton, S. Ciroi, E. Congiu, S. Chen,, and F. Di Mille

TL;DR
This paper reports the discovery of the largest double-sided relativistic jets in a spiral-hosted narrow-line Seyfert 1 galaxy, challenging previous beliefs about jet formation being exclusive to massive elliptical galaxies.
Contribution
It presents the first observation of extremely large, double-sided relativistic jets in a spiral-hosted NLS1 galaxy, demonstrating that powerful jets can originate from less massive black holes in spiral galaxies.
Findings
Largest double-sided jets in an NLS1 to date.
Jets extend nearly 250 kpc, larger than previously observed in similar galaxies.
Spiral galaxy host confirmed, challenging traditional jet-hosting galaxy models.
Abstract
Narrow-line Seyfert 1 (NLS1) galaxies are a peculiar subclass of active galactic nuclei (AGN). They have demonstrated that the presence of relativistic jets in an AGN is not strictly related to its radio-loudness, the black hole mass, or the host galaxy type. Here we present a remarkable example of a radio-quiet NLS1, 6dFGS gJ035432.8-134008 (J0354-1340). In our Karl G. Jansky Very Large Array observations at 5.5 GHz the source shows a bright core with a flat spectral index, and extended emission corresponding to very elongated jets. These are the largest double-sided radio jets found to date in an NLS1, with a deprojected linear size of almost 250 kpc. We also analysed near-infrared and optical images obtained by the Magellan Baade and the European Southern Observatory New Technology Telescope. By means of photometric decomposition and colour maps, we determined that J0354-1340 is…
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