Locating the warm absorber in NGC 4051

Details Locating the warm absorber in NGC 4051 Locating the warm absorber in NGC 4051

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009hrxs.confe..41s&link_type=abstract

"High Resolution X-ray Spectroscopy: Towards IXO, Proceedings of the international workshop held at the Mullard Space Science La

Physics

Scientific paper

I will present a detailed modeling of the Chandra LETGS spectrum taken
before, during and after the flux decreased by a factor of 5. The
resulting spectral changes and lack thereof allow us to place limits on
the location of the warm absorber. Using a previous LETGS spectrum we
locate 3 out of the 4 detected absorbers to be between 0.02 and 1 pc.

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