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We present an analysis of the properties of the hot interstellar medium (ISM)in the merging pair of galaxies known as The Antennae (NGC 4038/39), performedusing the deep, coadded ~411 ks Chandra ACIS-S data set. These deep X-rayobservations and Chandra's high angular resolution allow us to investigate theproperties of the hot ISM with unprecedented spatial and spectral resolution.Through a spatially resolved spectral analysis, we find a variety oftemperatures (from 0.2 to 0.7 keV) and Nh (from Galactic to 2x10^21 cm^-2).Metal abundances for Ne, Mg, Si, and Fe vary dramatically throughout the ISMfrom sub-solar values (~0.2) up to several times solar.Comment: 33 pages, 18 figures, revised version accepted by Astrophysical  Journal Supplement Serie

Chemical Enrichment of the Complex Hot ISM of the Antennae Galaxies. I. Spatial and Spectral Analysis of the Diffuse X‐Ray Emission