088168
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We propose a fulfill XMM-Newton programme to observe a sample of major mergers hosting AGN candidates based on their MIR WISE colours. Our goal is to characterise the X-ray emission in interacting galaxy pairs comma and to look for some possible interaction effects like offset nuclei comma or intermittent nuclear emission. We selected the galaxy pairs from the sample of Sekiguchi and Wolstencroft openPar1992MNRAS.255.581S comma SWclosePar comma of IR bright Arp-Madore major mergers.
创建时间:
2023-04-21



