Feedback by starbursts - the case of the missing link NGC4700
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While feedback on the ISM/IGM by nucleated starbursts is well understood anddescribed, it is less obvious how distributed starformation influences theISM/IGM connection and any associated large scale flow of matter. The target ofthis proposal, NGC4700, is a unique case with two regions of very intensivestarformation symmetric to the nucleus. The filamentary structure of the diffuseionized gas and the associated radiocontinuum emission suggest a high pressureof the ISM driving a large scale outflow. Xray observations with XMM/Newtonwill allow us to test this hypothesis and provide physical parameters importantto quantify feedback. Due to the unique morphology the target can be considereda missing link between nucleated and more distributed starbursts. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]



