VLBI Imaging of the X-ray Bright Lobe Hotspot in PKS B2152-699

Computer Science

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X-Ray, Radio, Dissipation Of Jets

Scientific paper

Wide-field very long baseline interferometric (VLBI) imaging can be used to study the compact radio structures in extended extragalactic radio sources such as starburst galaxies and radio galaxies. Recently, compact radio emission has been detected from the southern lobe hotspot in the nearby, powerful radio galaxy PKS B2152-699, using an array of Southern Hemisphere radio telescopes, resulting in the highest spatial resolution image of a radio galaxy hotspot to date. These VLBI data are being analyzed in conjunction with HST optical and Chandra X-ray observations to give a complete picture of the relationship between the relativistic jet in PKS B2152-699 and the host galaxy environment.

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