Modelling the broad-band spectra of X-ray emitting GPS galaxies

L. Ostorero, R. Moderski, Stawarz, M. C. Begelman, A. Diaferio, I. Kowalska, Jun Kataoka, S. J. Wagner

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

The study of the broad-band emission of GHz-Peaked-Spectrum (GPS) radio galaxies is a powerful tool to investigate the physical processes taking place in the central, kpc-sized region of their active hosts, where the jets propagate and the lobes expand, interacting with the surrounding interstellar medium (ISM). We recently developed a new dynamical-radiative model to describe the evolution of the GPS phenomenon (Stawarz et al. 2008): as the relativistic jets propagate through the ISM, gradually engulfing narrow-line emitting gas clouds along their way, the electron population of the expanding lobes evolves, emitting synchrotron light, as well as inverse-Compton radiation via up-scattering of the photon fields from the host galaxy and its active nucleus. The model, which successfully reproduces the key features of the GPS radio sources as a class, provides a description of the evolution of their spectral energy distribution (SED) with the lobes' expansion, predicting significant and complex X-ray to γ-ray emission. We apply here the model to the broad-band SED's of a sample of known, X-ray emitting GPS galaxies, and show that (i) the free-free absorption mechanism enables us to reproduce the radio continuum at frequencies below the turnover; (ii) the lobes' non-thermal, inverse-Compton emission can account for the observed X-ray spectra, providing a viable alternative to the thermal, accretion-dominated scenario. We also show that, in our sample, the relationship between the X-ray and radio hydrogen column densities, NH and NHI, is suggestive of a positive correlation, which, if confirmed, would support the scenario of high-energy emitting lobes.

Original languageEnglish
Pages (from-to)275-278
Number of pages4
JournalAstronomische Nachrichten
Volume330
Issue number2-3
DOIs
Publication statusPublished - 2009 Feb
Externally publishedYes

Fingerprint

lobes
galaxies
broadband
radio
modeling
x rays
radio galaxies
spectral energy distribution
energy
rays
turnover
synchrotrons
accretion
scattering
hydrogen
continuums
electron
nuclei
expansion
photons

Keywords

  • Active - galaxies
  • Galaxies
  • ISM - radiation mechanism
  • Jets - galaxies
  • Non-thermal
  • Nuclei - galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Ostorero, L., Moderski, R., Stawarz, Begelman, M. C., Diaferio, A., Kowalska, I., ... Wagner, S. J. (2009). Modelling the broad-band spectra of X-ray emitting GPS galaxies. Astronomische Nachrichten, 330(2-3), 275-278. https://doi.org/10.1002/asna.200811174

Modelling the broad-band spectra of X-ray emitting GPS galaxies. / Ostorero, L.; Moderski, R.; Stawarz; Begelman, M. C.; Diaferio, A.; Kowalska, I.; Kataoka, Jun; Wagner, S. J.

In: Astronomische Nachrichten, Vol. 330, No. 2-3, 02.2009, p. 275-278.

Research output: Contribution to journalArticle

Ostorero, L, Moderski, R, Stawarz, Begelman, MC, Diaferio, A, Kowalska, I, Kataoka, J & Wagner, SJ 2009, 'Modelling the broad-band spectra of X-ray emitting GPS galaxies', Astronomische Nachrichten, vol. 330, no. 2-3, pp. 275-278. https://doi.org/10.1002/asna.200811174
Ostorero L, Moderski R, Stawarz, Begelman MC, Diaferio A, Kowalska I et al. Modelling the broad-band spectra of X-ray emitting GPS galaxies. Astronomische Nachrichten. 2009 Feb;330(2-3):275-278. https://doi.org/10.1002/asna.200811174
Ostorero, L. ; Moderski, R. ; Stawarz ; Begelman, M. C. ; Diaferio, A. ; Kowalska, I. ; Kataoka, Jun ; Wagner, S. J. / Modelling the broad-band spectra of X-ray emitting GPS galaxies. In: Astronomische Nachrichten. 2009 ; Vol. 330, No. 2-3. pp. 275-278.
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