Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182..661c&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 182, Mar. 1978, p. 661-671.
Astronomy and Astrophysics
Astronomy
20
Compton Effect, Radio Sources (Astronomy), Satellite Observation, Spaceborne Astronomy, X Ray Sources, Ariel 5 Satellite, Background Radiation, Electron Radiation, Magnetic Fields, Microwave Emission, Sky Surveys (Astronomy)
Scientific paper
The University of Leicester Sky Survey Instrument on the Ariel V X-ray astronomy satellite has detected, at high statistical significance, spatially extended X-ray emission from the giant radio lobes of Cen A. The combined emission of both lobes amounts to 1.3 (plus or minus 0.18) x 10 to the -10 erg/sq cm/s (2-10 keV), which corresponds to 3.7 x 10 to the 41 erg/s at a distance of 5 Mpc. Interpreting the X-rays as Inverse Compton Scattered photons of the microwave background by the radio-emitting electrons, we estimate the average strength of the magnetic field to be 0.7 microgauss, a value almost equal to the equipartition value computed with protons having the same energy content as electrons. There is strong evidence that the peaks of the X-ray emission do not coincide with the radio peaks but are further from the galaxy. This indicates that probably the magnetic field strength decreases by a factor 2-3 along the lobes away from the galaxy, whereas the electron density appears to be larger away from the galaxy than close to it.
Cooke Brin A.
Lawrence Andy
Perola Giuseppe Cesare
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