XMM-Newton Proposal 03025701

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Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Baade'S Foregro, Xmm-Newton Proposal 03025701

Scientific paper

This proposal is a request for the reobservation of an AO-3 target for which a 25 ks exposure was almost entirely contaminated by strong soft proton flares, and thus cannot be used to meet our scientific objectives. This exposure is the linch-pin to the analysis of the other observations in this program; without the reobservation, the interpretation of the other observations will be equivocal. We will be measuring the temperature of soft components of the Galactic X-ray bulge as close to the nucleus as possible, through Baade's Window. We will then measure the change in temperature with distance from the nucleus. From these measures we expect to determine the thermal history of the gas in the X-ray emitting bulge and thus the impact of the central engine.

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