Loading…
Simulations of two-temperature jets in galaxy clusters: II. X-ray properties of the forward shock
Context. Forward shocks by radio jets, driven into the intracluster medium, are one of the indicators that can be used to evaluate the power of the jet. Meanwhile, high-angular-resolution X-ray observations show the Mach numbers of powerful radio jets are smaller compared to the results of theoretic...
Saved in:
Published in: | Astronomy and astrophysics (Berlin) 2023-11, Vol.679, p.A161 |
---|---|
Main Authors: | , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | Context.
Forward shocks by radio jets, driven into the intracluster medium, are one of the indicators that can be used to evaluate the power of the jet. Meanwhile, high-angular-resolution X-ray observations show the Mach numbers of powerful radio jets are smaller compared to the results of theoretical and numerical studies, namely, ℳ
obs
|
---|---|
ISSN: | 0004-6361 1432-0746 |
DOI: | 10.1051/0004-6361/202244692 |