Multiple X-ray emission components in low-power radio galaxies

Details Multiple X-ray emission components in low-power radio galaxies Multiple X-ray emission components in low-power radio galaxies

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...427..134w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 427, no. 1, p. 134-139

Astronomy and Astrophysics

Astronomy

80

Data Reduction, Elliptical Galaxies, Radio Jets (Astronomy), Spectrum Analysis, X Rays, Astronomical Observatories, Line Of Sight, Luminosity, Radio Emission, Rosat Mission

Scientific paper

We report x-ray observations of the first six sources observed with ROSAT in our study of low-power radio galaxies. Spatial and spectral measurements show that both resolved (thermal) and unresolved X-ray emission in a single source are typical, although the relative strength and size of the resolved component varies between objects. The unresolved X-ray component correlates well with the core radio emission and may be dominated by nonthermal emission associated with an inner radio jet.

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