Virial clouds explaining the observed rotational asymmetry in the galactic halos
Virial clouds explaining the observed rotational asymmetry in the galactic halos
Rotation of galactic objects has been seen in the cosmic microwave background (CMB) that could be ascribed to molecular hydrogen clouds with, or without, dust contamination and contamination from other sources. We model the clouds using the canonical ensemble for pure molecular hydrogen, a mixture of hydrogen helium and/or dust, …