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XMM-Newton Survey of the Magellanic Bridge
We aim to characterise the X-ray binary population as a function of the local stellar population (in terms of age, metallicity, and stellar density) in the Magellanic Bridge, the interconnecting region between the Small and Large Magellanic Cloud. Gardiner and Noguchi (1996) suggest that closest app...
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| Language: | English |
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Department of Astronomy
2021
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