The Radio Lobe/ICM Interaction in the Unusual Radio Galaxy 3C 310

Details The Radio Lobe/ICM Interaction in the Unusual Radio Galaxy 3C 310 The Radio Lobe/ICM Interaction in the Unusual Radio Galaxy 3C 310

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2947m&link_type=abstract

Chandra proposal ID #11700016

Computer Science

Scientific paper

We propose a 60 ks observation of the hot gas around the unusual double-lobed radio galaxy 3C 310 to constrain the dynamics of the gas interaction with the radio bubbles. The radio emission from the lobes of 3C 310 show a variety of shells and filaments embedded within a larger scale diffuse emission. The southern lobe had a bright ring in the center, similar to the one seen in Her A, that may be the result of a complex interaction between the buoyant bubble and the ICM. Two merging elliptical galaxies lie at the center of the cluster gas. This observation will permit us to determine what effect that dynamic cluster gas, stirred up from the merger, had on the evolution of the radio bubble.

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