THE JET HEATED X-RAY FILAMENT IN THE CENTAURUS A NORTHERN MIDDLE RADIO LOBE

R. P. Kraft*, W. R. Forman, M. J. Hardcastle, M. Birkinshaw, J. H. Croston, C. Jones, P. E. J. Nulsen, D. M. Worrall, S. S. Murray

*Corresponding author for this work

Research output: Contribution to journalArticle (Academic Journal)peer-review

42 Citations (Scopus)

Abstract

We present results from a 40 ks XMM-Newton observation of the X-ray filament coincident with the southeast edge of the Centaurus A Northern Middle Radio Lobe (NML). We find that the X-ray filament consists of five spatially resolved X-ray knots embedded in a continuous diffuse bridge. The spectrum of each knot is well fitted by a thermal model with temperatures ranging from 0.3 to 0.7 keV and subsolar elemental abundances. In four of the five knots, nonthermal models are a poor fit to the spectra, conclusively ruling out synchrotron or IC/CMB mechanisms for their emission. The internal pressures of the knots exceed that of the ambient interstellar medium or the equipartition pressure of the NML by more than an order of magnitude, demonstrating that they must be short lived (similar to 3 x 10(6) yr). Based on energetic arguments, it is implausible that these knots have been ionized by the beamed flux from the active galactic nucleus of Cen A or that they have been shock heated by supersonic inflation of the NML. In our view, the most viable scenario for the origin of the X-ray knots is that they are the result of cold gas shock heated by a direct interaction with the jet. The most plausible model of the NML is that it is a bubble from a previous nuclear outburst that is being re-energized by the current outburst. The northeast inner lobe and the large-scale jet are lossless channels through which the jet material rapidly travels to the NML in this scenario. We also report the discovery of a large-scale (at least 35 kpc radius) gas halo around Cen A.

Original languageEnglish
Pages (from-to)2036-2047
Number of pages12
JournalAstrophysical Journal
Volume698
Issue number2
DOIs
Publication statusPublished - 20 Jun 2009

Keywords

  • hydrodynamics
  • galaxies: individual (Centaurus A, NGC 5128)
  • galaxies: jets
  • X-rays: galaxies
  • HOT INTERSTELLAR-MEDIUM
  • HUBBLE-SPACE-TELESCOPE
  • INDUCED STAR-FORMATION
  • NGC 5128
  • CLOUD INTERACTIONS
  • OPTICAL FILAMENTS
  • GALAXY NGC-2110
  • IONIZED-GAS
  • A EVIDENCE
  • CHANDRA

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