Halos and clusters #534
Lucia-Fonseca
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Halos and clusters
#534
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@sutieng would you have any suggestion? |
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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. |
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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!
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