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Open AccessArticle10.1051/0004-6361/201425442

Redshifted Fe K<i>α</i>line from the unusual<i>γ</i>-ray source PMN J1603–4904

C. Müller,F. Krauß,T. Dauser,A. Kreikenbohm,T. Beuchert,M. Kadler+10 more-2015-01-13-Astronomy and Astrophysics
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TL;DRAbstract

Context. Multiwavelength observations have revealed the highly unusual properties of the γ-ray source PMN J1603–4904, which are difficult to reconcile with any other well-established γ-ray source class. The object is either a very atypical blazar or a compact jet source seen at a larger angle to the line of sight.

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Context. Multiwavelength observations have revealed the highly unusual properties of the γ-ray source PMN J1603–4904, which are difficult to reconcile with any other well-established γ-ray source class. The object is either a very atypical blazar or a compact jet source seen at a larger angle to the line of sight.

Keywords

RedshiftBlazarQuasarLine (geometry)Emission spectrumBL Lac objectSpectral lineJet (fluid)

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