Do the Herschel cold clouds in the Galactic halo embody its dark matter?
Theo M. Nieuwenhuizen, Erik F. G. van Heusden, Matthew T. P. Liska

TL;DR
This paper proposes that Herschel cold clouds observed in the Magellanic Clouds are Jeans clusters of dark matter, potentially accounting for the Galaxy's missing mass and baryons, based on their size, mass, and distribution.
Contribution
It introduces a model linking Herschel cold clouds to Jeans clusters, suggesting they constitute all Galactic dark matter and baryons, supported by observational data and theoretical analysis.
Findings
Herschel cold clouds have a radius of about 2.5 pc.
HCCs could account for all the missing Galactic halo mass.
Jeans clusters may contain billions of MACHOs of Earth mass.
Abstract
Recent Herschel/SPIRE maps of the Small and Large Magellanic Clouds (SMC, LMC) exhibit in each thousands of clouds. Observed at 250 microns, they must be cold, T ~ 15 K, hence the name "Herschel cold clouds" (HCCs). From the observed rotational velocity profile and the assumption of spherical symmetry, the Galactic mass density is modeled in a form close to that of an isothermal sphere. If the HCCs constitute a certain fraction of it, their angular size distribution has a specified shape. A fit to the data deduced from the SMC/LMC maps supports this and yields for their radius 2.5 pc, with a small change when allowing for a spread in HCC radii. There are so many HCCs that they will make up all the missing Halo mass density if there is spherical symmetry and their average mass is of order 15,000 Mo. This compares well with the Jeans mass of circa 40,000 Mo and puts forward that the HCCs…
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