X-RAY-EMITTING GHz-PEAKED-SPECTRUM GALAXIES: TESTING A DYNAMICAL-RADIATIVE MODEL WITH BROADBAND SPECTRA
- Dipartimento di Fisica Generale 'Amedeo Avogadro', Universita degli Studi di Torino, Via P. Giuria 1, 10125 Torino (Italy)
- Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw (Poland)
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305 (United States)
- Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warsaw (Poland)
- NASA Goddard Space Flight Center, Astrophysics Science Division, Greenbelt, MD 20771 (United States)
- Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan)
- Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, CO 80309-0440 (United States)
- Landessternwarte Heidelberg-Koenigstuhl, Koenigstuhl 12, 69117 Heidelberg (Germany)
In a dynamical-radiative model we recently developed to describe the physics of compact, GHz-peaked-spectrum (GPS) sources, the relativistic jets propagate across the inner, kpc-sized region of the host galaxy, while the electron population of the expanding lobes evolves and emits synchrotron and inverse-Compton (IC) radiation. Interstellar-medium gas clouds engulfed by the expanding lobes, and photoionized by the active nucleus, are responsible for the radio spectral turnover through free-free absorption (FFA) of the synchrotron photons. The model provides a description of the evolution of the spectral energy distribution (SED) of GPS sources with their expansion, predicting significant and complex high-energy emission, from the X-ray to the {gamma}-ray frequency domain. Here, we test this model with the broadband SEDs of a sample of 11 X-ray-emitting GPS galaxies with compact-symmetric-object morphology, and show that (1) the shape of the radio continuum at frequencies lower than the spectral turnover is indeed well accounted for by the FFA mechanism and (2) the observed X-ray spectra can be interpreted as non-thermal radiation produced via IC scattering of the local radiation fields off the lobe particles, providing a viable alternative to the thermal, accretion-disk-dominated scenario. We also show that the relation between the hydrogen column densities derived from the X-ray (N {sub H}) and radio (N {sub HI}) data of the sources is suggestive of a positive correlation, which, if confirmed by future observations, would provide further support to our scenario of high-energy emitting lobes.
- OSTI ID:
- 21450917
- Journal Information:
- Astrophysical Journal, Vol. 715, Issue 2; Other Information: DOI: 10.1088/0004-637X/715/2/1071; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
COSMOLOGY AND ASTRONOMY
ACCRETION DISKS
ENERGY SPECTRA
GALACTIC EVOLUTION
GAMMA RADIATION
HYDROGEN
PHOTOIONIZATION
PHOTONS
RELATIVISTIC RANGE
X-RAY GALAXIES
X-RAY SPECTRA
BOSONS
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ELEMENTS
ENERGY RANGE
EVOLUTION
GALAXIES
IONIZATION
IONIZING RADIATIONS
MASSLESS PARTICLES
NONMETALS
RADIATIONS
SPECTRA