Halos and clusters #534
Lucia-Fonseca
started this conversation in
Ideas
Halos and clusters
#534
Replies: 1 comment 1 reply
-
|
@sutieng would you have any suggestion? |
Beta Was this translation helpful? Give feedback.
1 reply
-
|
The current halo module has already implemented some characteristic DM properties for cluster-scale halos by assuming NFW model. For the baryonic component, to obtain the full X-ray brightness distribution, it would require some hydrodynamical simulations. Alternatively, we could use scaling relations to connect DM with baryons, and paint each sampled NFW halo with X-ray properties. |
Beta Was this translation helpful? Give feedback.
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment
Uh oh!
There was an error while loading. Please reload this page.
-
Halos and clusters: next step: feature of baryonic component in galaxy cluster, e.g. X-ray luminosity, X-ray temperature, gas mass.
@sutieng please feel free to add any more information to this topic. Thanks!
Beta Was this translation helpful? Give feedback.
All reactions