The Future for Warm Absorbers

Details The Future for Warm Absorbers The Future for Warm Absorbers

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006hrxs.confe...2b&link_type=abstract

High Resolution X-ray Spectroscopy: towards XEUS and Con-X, Proceedings of the international workshop held at the Mullard Space

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It has been a good five years for those who study warm absorbers - outflows of ionised gas from AGN - due to the multitude of excellent high-resolution soft X-ray spectra delivered by XMM-Newton and Chandra. We now have a far better understanding of the absorbing columns, ionisation range and origins of the outflows. But where do we go from here? In this presentation I discuss the potential cosmological importance of warm absorber outflows, a future direction the field could take, and what we will need from future missions in order to get there.

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