Date Presented:

2013/09/1

Abstract:

Nearby galaxies are well suited for investigating X-ray source populations in different environments than in our own Galaxy. Moreover, sources in these galaxies have well determined distances and are less absorbed than sources in the galactic plane. The Large (LMC) and the Small (SMC) Magellanic Clouds (MC) are the nearest gas-rich star-forming galaxies and their gravitational interactions are believed to have tidally triggered recent bursts of star formation. The XMM-Newton large program for the SMC, together with archival observations covers an area of 5.5 square degrees and has already produced significant results. The XMM-Newton large program for the LMC has just been completed and has covered an even bigger area of about 10 square degrees. Both surveys reach a limiting luminosity of 1032 erg/s and provide a unique data set for X-ray source population studies. The two surveys have allowed us to derive hardness ratios for the point sources and conduct spectral classification. For the brightest sources, we performed spectral and timing analysis. By complementing these results with surveys at other wavelengths we have managed to extend our understanding of the nature of individual sources as well as providing complete data-sets of X-ray source populations (X-ray Binaries, supersoft sources, supernova remnants, background active galactic nuclei and foreground galactic sources). From the classification of the sources we have constructed luminosity functions which will allow as to compare X-ray populations in the different environments that the MCs provide. Here, we present an overview of these two surveys together with the highlights of the most interesting sources that they have produced so far (e.g. Be/X-ray binaries).

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