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A disk-dominated and clumpy circumgalactic medium of the Milky Way seen in X-ray emission

Soft X-ray observations of the southern Galactic sky with the HaloSat CubeSat indicate that the circumgalactic medium (CGM) of the Milky Way has a disk-like profile, with an extended spherical halo. Clumps in the CGM correlate with star-formation activity.

P. Kaaret
D. Koutroumpa
A. Zajczyk
Research19 Oct 2020
Nature Astronomy

Volume: 4, P: 1072-1077

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A disk-dominated and clumpy circumgalactic medium of the Milky Way seen in X-ray emission

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