The X-ray view of giga-hertz peaked spectrum radio galaxies

O. Tengstrand*, M. Guainazzi, A. Siemiginowska, N. Fonseca Bonilla, A. Labiano, D. M. Worrall, P. Grandi, E. Piconcelli

*Corresponding author for this work

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

41 Citations (Scopus)

Abstract

Context. This paper presents the X-ray properties of a flux- and volume-limited complete sample of 16 giga-hertz peaked spectrum (GPS) galaxies.

Aims. This study addresses three basic questions in our understanding of the nature and evolution of GPS sources: a) What is the physical origin of the X-ray emission in GPS galaxies? b) Which physical system is associated with the X-ray obscuration? c) What is the "endpoint" of the evolution of compact radio sources?

Methods. We discuss in this paper the results of the X-ray spectral analysis, and compare the X-ray properties of the sample sources with radio observables.

Results. We obtain a 100% (94%) detection fraction in the 0.5-2 keV (0.5-10 keV) energy band. GPS galaxy X-ray spectra are typically highly obscured (<N(H)(GPS)> = 3 x 10(22) cm(-2); sigma(NH) similar or equal to 0.5 dex). The X-ray column density is larger than the HI column density measured in the radio by a factor 10 to 100. GPS galaxies lie well on the extrapolation to high radio powers of the correlation between radio and X-ray luminosity known in low-luminosity FR I radio galaxies. On the other hand, GPS galaxies exhibit a comparable X-ray luminosity to FR II radio galaxies, notwithstanding their much larger radio luminosity.

Conclusions. The X-ray to radio luminosity ratio distribution in our sample is consistent with the bulk of the high-energy emission being produced by the accretion disk, as well as with dynamical models of GPS evolution where X-rays are produced by Compton upscattering of ambient photons. Further support to the former scenario comes from the location of GPS galaxies in the X-ray to O[III] luminosity ratio versus N(H) plane. We propose that GPS galaxies are young radio sources, which would reach their full maturity as classical FR II radio galaxies. However, column densities greater than or similar to 10(22) cm(-2) could lead to a significant underestimate of dynamical age determinations based on the hotspot recession velocity measurements.

Original languageEnglish
Pages (from-to)89-102
Number of pages14
JournalAstronomy and Astrophysics
Volume501
Issue number1
DOIs
Publication statusPublished - Jul 2009

Keywords

  • galaxies: jets
  • galaxies: active
  • X-rays: galaxies
  • COMPACT STEEP-SPECTRUM
  • ACTIVE GALACTIC NUCLEI
  • PHOTON IMAGING CAMERA
  • DIGITAL SKY SURVEY
  • COMPTON-THICK AGN
  • HI ABSORBING GAS
  • XMM-NEWTON
  • SYMMETRIC OBJECTS
  • FR-I
  • ENERGY-DISTRIBUTIONS

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