HIGHLIGHTS
SUMMARY
The suggestion had been to consider the sister galaxy Andromeda (M31), and assume that the clouds rotate with the whole M31 halo. The authors now use a more reliable model described in detail in Ref to estimate the physical parameters of virial clouds with contamination of halo dust grains in them. Virial Cloud Model Virial clouds populating the galactic halos are assumed to be spherically symmetric and at a temperature equal to that of the CMB, i.e., T ` 2.7 K. Each cloud is assumed to be composed of molecular hydrogen, helium, and . . .
If you want to have access to all the content you need to log in!
Thanks :)
If you don't have an account, you can create one here.