A Multiwavelength Study of the Extreme AGN J2310-437
arXiv:astro-ph/9808027 · doi:10.1086/307074
Abstract
We present new X-ray, radio, and optical data for the unusual galaxy/cluster system J2310-437. Our results confirm the presence of an active nucleus, and suggest an interpretation as an anomalous BL Lac object of bulk relativistic Doppler factor < 2, with an optically deficient radio-to-X-ray spectrum. The radio, optical, and soft X-ray flux densities could lie along a single power-law function, lacking the curvature typical of BL Lac objects. Compared with other known sources that may have comparable multifrequency spectra, J2310-437 is the most extreme. Its low isotropic optical/UV radiation is consistent with the intensity of external photons governing the electron spectral break through Compton cooling; in this source the external photon density would be too low to produce a spectral break below the X-ray.
arXiv comment19 pages, including 10 figures, using emulateapj.sty and apjfonts.sty. To appear in the ApJ
References in corpus (4)
Cited by in corpus (9)
- The Extended Chandra Deep Field-South Survey: Optical spectroscopy of faint X-ray sources with the VLT and Keck
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- A Multiwavelength Spectral and Polarimetric Study of the Jet of 3C 264
- Separating the BL Lac and Cluster X-ray Emissions in Abell 689 with Chandra
- The Knotty Question of the Jet of PKS B1421-490
- The Gaseous Environments of Radio Galaxies
- Unmasking the Active Galactic Nucleus in PKS J2310-437