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authorAaron LI <aly@aaronly.me>2017-10-14 10:21:07 +0800
committerAaron LI <aly@aaronly.me>2017-10-14 10:21:07 +0800
commit62a6a5a15a759da45cec210babbca52ca27a25b5 (patch)
treec56cf6f99a9a240397dd08fb479647620315dda4 /fg21sim/extragalactic/clusters/main.py
parentf29de49b06f1ac0bcee1b3a3f763888afe2ac8b4 (diff)
downloadfg21sim-62a6a5a15a759da45cec210babbca52ca27a25b5.tar.bz2
clusters: Update the documents/comments a b it
Diffstat (limited to 'fg21sim/extragalactic/clusters/main.py')
-rw-r--r--fg21sim/extragalactic/clusters/main.py13
1 files changed, 4 insertions, 9 deletions
diff --git a/fg21sim/extragalactic/clusters/main.py b/fg21sim/extragalactic/clusters/main.py
index a5c2497..7149f69 100644
--- a/fg21sim/extragalactic/clusters/main.py
+++ b/fg21sim/extragalactic/clusters/main.py
@@ -2,19 +2,14 @@
# MIT license
"""
-Simulate the extended radio emissions from the galaxy cluster,
-e.g., giant radio halos, radio relics.
+Simulate the extended radio emissions from galaxy clusters due to
+merger-induced turbulence and/or shock accelerations,
+e.g., (giant) radio halos, (elongated double) radio relics.
NOTE
----
There are other types of extended radio emissions not considered
yet, e.g., mini-halos, roundish radio relics, etc.
-
-References
-----------
-.. [cassano2012]
- Cassano et al. 2012, A&A, 548, A100
- http://adsabs.harvard.edu/abs/2012A%26A...548A.100C
"""
import os
@@ -175,7 +170,7 @@ class GalaxyClusters:
NOTE
----
There may be no such recent major merger event satisfying the
- criteria, since we only tracing ``tau_merger`` (~3 Gyr) back.
+ criteria, since we only tracing ``tau_merger`` (~2-3 Gyr) back.
On the other hand, the cluster may only experience minor merger
or accretion events.