Volume 426, Number 3, November II 2004
|Page(s)||777 - 777|
|Section||Cosmology (including clusters of galaxies)|
|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: firstname.lastname@example.org
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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