A giant radio jet ejected by an ultramassive black hole in a single-lobed radio galaxy
arXiv:0712.0543 · doi:10.1086/524220
Abstract
We report the discovery of a very unusual, highly asymmetric radio galaxy whose radio jet, the largest yet detected, emits strongly polarized synchrotron radiation and can be traced all the way from the galactic nucleus to the hot spot located ~440 kpc away. This jet emanates from an extremely massive black hole (>10^9 solar mass) and forms a strikingly compact radio lobe. No radio lobe is detected on the side of the counterjet, even though it is similar to the main jet in brightness up to a scale of tens of kiloparsecs. Thus, contrary to the nearly universal trend, the brightness asymmetry in this radio galaxy increases with distance from the nucleus. With several unusual properties, including a predominantly toroidal magnetic field, this Fanaroff-Riley type II megajet is an exceptionally useful laboratory for testing the role of magnetic field in jet stabilization and radio lobe formation.
Published in The Astrophysical Journal Letters, Volume 670, L85-L88, 2007
References in corpus (5)
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- A new list of extra-galactic radio jets
- On the Jet Activity in 3C 273
- Confronting X-ray Emission Models with the Highest-Redshift Kiloparsec-scale Jets: the z=3.89 Jet in Quasar 1745+624
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- Low-frequency High-resolution Radio Observations of the TeV-emitting Blazar SHBLJ001355.9-185406
- A (likely) X-ray jet from NGC6217 observed by XMM-Newton