Feedback by starbursts - the case of the missing link NGC4700

Details Feedback by starbursts - the case of the missing link NGC4700 Feedback by starbursts - the case of the missing link NGC4700

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...96d&link_type=abstract

XMM-Newton Proposal ID #05530301

Physics

Galaxies, Galactic Surveys, Ngc4700, Xmm-Newton Proposal Id #05530301

Scientific paper

While feedback on the ISM/IGM by nucleated starbursts is well understood and described, it is less obvious how distributed starformation influences the ISM/IGM connection and any associated large scale flow of matter. The target of this proposal, NGC4700, is a unique case with two regions of very intensive starformation symmetric to the nucleus. The filamentary structure of the diffuse ionized gas and the associated radiocontinuum emission suggest a high pressure of the ISM driving a large scale outflow. X-ray observations with XMM/Newton will allow us to test this hypothesis and provide physical parameters important to quantify feedback. Due to the unique morphology the target can be considered a missing link between nucleated and more distributed starbursts.

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