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Jet and accretion-disk emission untangled in 3C 273

Paola Grandi1, Giorgio G C Palumbo

  • 1Istituto di Astrofisica Spaziale e Fisica Cosmica, Consiglio Nazionale delle Ricerche-Istituto Nazionale di Astrofisica, Sezione di Bologna, Via Gobetti 101, I-40129, Bologna, Italy. grandi@bo.iasf.cnr.it

Science (New York, N.Y.)
|November 6, 2004
PubMed
Summary

This study of active galactic nucleus 3C 273 reveals that jet power increases with energy. The nonthermal jet radiation typically overwhelms thermal accretion flow emission, except when an iron line becomes visible.

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