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Highly Polarized Emission from the E-Hotspot in DA240

Published online by Cambridge University Press:  14 August 2015

S. C. Tsien
Affiliation:
Mullard Radio Astronomy Observatory, Cambridge
Richard Saunders
Affiliation:
Mullard Radio Astronomy Observatory, Cambridge

Extract

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The hotspot in the eastern lobe of the nearby giant radio galaxy DA240 (z=0.0356) provides a rare opportunity to examine the detailed polarization structure of a hotspot. Maps have been made with the Cambridge 5-km telescope at 2.7 and 5.0 GHz. The 5.0-GHz maps are shown in Figs 1 and 2. The main characteristics are: (a) The hotspot has an overall size in the 2.7-GHz map of 10×18 kpc2. It blends smoothly at its outer edge into the background of the extended lobe. The 5.0 GHz total intensity map shows a yet more compact region (subcomponent A). It has not been fully resolved in the direction of the minor axis and has a size <1×2.5 kpc2. There is a second much weaker and diffuse region (subcomponent B). Both subcomponents are superimposed on a broad plateau of emission. The hotspot has spectral index α(0.61–5.0)=0.52, minimum total energy Emin=3×1056 ergs and equipartition magnetic field Beq=2×10−5 G, values typical of other hotspots, although its projected distance from the nucleus is very large (0.65 Mpc);

Type
Research Article
Copyright
Copyright © Reidel 1982