The puzzling iron line emission of ESO198-G24

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Chandra Proposal Id #05700512

Scientific paper

We propose to observe with Chandra ACIS-S HETG the Seyfert 1 Galaxy ESO198-G24 for 150 ks. ESO198-G24 has a very puzzling iron line complex, composed by a 6.4 keV line with a variable profile and a narrow component at a lower energy (5.7 keV and 5.9 keV in the two XMM-Newton observations), reminiscent of similar features observed in NGC 3516. Our proposal aims to shed more light on the origin of these features by better constraning their intrinsic width.

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