Diffuse Neutral Hydrogen in the Local Group

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The close proximity of the Local Group galaxy M31 provides us with the opportunity to study its surrounding circumgalactic medium and the intergalactic medium in detail. I will present my research on mapping and analysing the diffuse neutral hydrogen gas (HI) that exists within Local Group. I will discuss the discovery and possible origins of HI clouds that lie between the galaxies M31 and M33 as well as the faint HI now confirmed to the northwest of M31. I will also briefly summarize our ongoing and planned future work.

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