| Issue |
A&A
Volume 426, Number 3, November II 2004
|
|
|---|---|---|
| Page(s) | 777 - 777 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361:20041826 | |
| Published online | 18 October 2004 | |
Constraining the population of cosmic ray protons in cooling flow clusters with γ-ray and radio observations: Are radio mini-halos of hadronic origin?
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str.1, Postfach 1317, 85741 Garching, Germany e-mail: pfrommer@mpa-garching.mpg.de
This article has no abstract.
Key words: errata, addenda / galaxies: cooling flows / galaxies: clusters: general / galaxies: clusters: individual: Perseus (A426) / radiation mechanisms: non-thermal
© ESO, 2004
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