Detection of Gamma Rays from a Starburst Galaxy

Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of approximately 10¹⁵ electron volts. We report the detection of gamma rays--tracers of such cosmic rays--from the starburst...

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Veröffentlicht in:Science (American Association for the Advancement of Science) 2009-11, Vol.326 (5956), p.1080-1082
Hauptverfasser: Acero, F, Akhperjanian, A.G, Anton, G, Barres de Almeida, U, Bazer-Bachi, A.R, Behera, B, Bochow, A, Boisson, C, Borrel, V, Brucker, J, Brun, F, Bühler, R, Charbonnier, A, Chaves, R.C.G, Cheesebrough, A, Chounet, L.-M, Clapson, A.C, Coignet, G, Davids, I.D, Deil, C, Dickinson, H.J, Djannati-Ataï, A, Domainko, W, Drury, L. O'C, Dubus, G, Dyrda, M, Egberts, K, Emmanoulopoulos, D, Fegan, S, Feinstein, F, Fiasson, A, Fontaine, G, Füssling, M, Gabici, S, Gallant, Y.A, Gérard, L, Gerbig, D, Giebels, B, Göring, D, Hauser, D, Hauser, M, Henri, G, Hermann, G, Hinton, J.A, Hofverberg, P, Hoppe, S, de Jager, O.C, Katarzyński, K, Katz, U, Kaufmann, S, Kerschhaggl, M, Khangulyan, D, Klochkov, D, Kneiske, T, Komin, Nu, Kosack, K, Kossakowski, R, Lenain, J.-P, Lohse, T, Marcowith, A, Masbou, J, McComb, T.J.L, Medina, M.C, Moderski, R, Moulin, E, de Naurois, M, Niemiec, J, Ohm, S, Olive, J.F, Orford, K.J, Ostrowski, M, Petrucci, P.-O, Pita, S, Raubenheimer, B.C, Raue, M, Rieger, F, Ripken, J, Rosier-Lees, S, Rowell, G, Rudak, B, Rulten, C.B, Ruppel, J, Sahakian, V, Santangelo, A, Schlickeiser, R, Schwanke, U, Schwarzburg, S, Sol, H, Stawarz, Ł, Szostek, A, Terrier, R, Tluczykont, M, van Eldik, C, Venter, C, Venter, L, Vialle, J.P, Volpe, F, Wagner, S.J, Ward, M, Zdziarski, A.A
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Sprache:eng
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Zusammenfassung:Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of approximately 10¹⁵ electron volts. We report the detection of gamma rays--tracers of such cosmic rays--from the starburst galaxy NGC 253 using the High Energy Stereoscopic System (H.E.S.S.) array of imaging atmospheric Cherenkov telescopes. The gamma-ray flux above 220 billion electron volts is F = (5.5 ± 1.0stat ± 2.8sys) x 10⁻¹³ cm⁻² s⁻¹, implying a cosmic-ray density about three orders of magnitude larger than that in the center of the Milky Way. The fraction of cosmic-ray energy channeled into gamma rays in this starburst environment is five times as large as that in our Galaxy.
ISSN:0036-8075
1095-9203
1095-9203
DOI:10.1126/science.1178826