On the Galactic Halos Rotation by <i>Planck</i> Data
As galactic halos are not directly visible, there are many ambiguities regarding their composition and rotational velocity. Though most of the dark matter is non-baryonic, <i>some fraction is</i>, and it can be used to trace the halo rotation. Asymmetries in the CMB towards M31 had been...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2023-01-01
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| Series: | Symmetry |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2073-8994/15/1/160 |