Volume 407, Number 3, September I 2003
|Page(s)||L73 - L77|
|Published online||17 November 2003|
Letter to the Editor
Probing the cosmic ray population of the giant elliptical galaxy M 87 with observed TeV γ-rays
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str.1, Postfach 1317, 85741 Garching, Germany
Corresponding author: C. Pfrommer, firstname.lastname@example.org
Accepted: 15 July 2003
We examine the cosmic ray proton (CRp) population within the giant elliptical galaxy M 87 using the TeV γ-ray detection of the HEGRA collaboration. In our scenario, the γ-rays are produced by decaying pions which result from hadronic CRp interactions with thermal gas of the interstellar medium of M 87. By comparing the γ-ray emission to upper limits from EGRET, we constrain the spectral index of the CRp population to within our scenario. Both the expected radial γ-ray profile and the required amount of CRp support this hadronic scenario. The accompanying radio mini-halo of hadronically originating cosmic ray electrons is outshone by the synchrotron emission of the relativistic jet of M 87 by one order of magnitude. According to our predictions, the future GLAST mission should allow us to test this hadronic scenario.
Key words: γ-rays: theory / cosmic rays / galaxies: individual: M 87 / galaxies: cooling flows / intergalactic medium / radiation mechanisms: non-thermal
© ESO, 2003
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