The nature of the variable X-ray absorber in ESO 362-G18

Physics

Scientific paper

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Scientific paper

We propose a monitoring program of ESO 362-G18, a X-ray bright local Seyfert 1.5 which exhibits significant variation of the properties of the X-ray absorber on relatively short timescales. We identify a likely variability timescale of 1 week, and we propose to monitor the source for 2 weeks and explore all shorter timescales by making use of Chandra and XMM-Newton unique capabilities. We request a total of 5x10 ks time-constrained observations with Chandra and 1x75 ks unconstrained observation with XMM-Newton.

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