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Autor:
Ajello, and Baldini, M., and Barbiellini, L., and Bastieri, G., and Bellazzini, D., and Bissaldi, R., and Bloom, E., and Bonino, E. D., and Bottacini, R., and Brandt, E., and Bregeon, T. J., and Bruel, J., and Buehler, P., and Caliandro, R., and Cameron, G. A., and Caragiulo, R. A., and Cavazzuti, M., and Charles, E., and Chekhtman, E., and Ciprini, A., and Cohen-Tanugi, S., and Condon, J., and Costanza, B., and Cutini, F., and D'Ammando, S., and Palma, F., and Desiante, F. D., and Lalla, R., and Mauro, N. D., and Venere, M. D., and Drell, L. D., and Dubner, P. S., and Dumora, G., and Duvidovich, D., and Favuzzi, L., and Focke, C., and Fusco, W. B., and Gargano, P., and Gasparrini, F., and Giacani, D., and Giglietto, E., and Glanzman, N., and Green, T., and Grenier, D. A., and Guiriec, I. A., and Hays, S., and Hewitt, E., and Hill, J. W., and Horan, A. B., and Jogler, D., and Jóhannesson, T., and Jung-Richardt, G., and Kensei, I., and Kuss, S., and Larsson, M., and Latronico, S., and Lemoine-Goumard, L., and Li, M., and Li, J., and Longo, L., and Loparco, F., and Lovellette, F., and Lubrano, M. N., and Magill, P., and Maldera, J., and Manfreda, S., and Mayer, A., and Mazziotta, M., and McEnery, M. N., and Michelson, J. E., and Mitthumsiri, P. F., and Mizuno, W., and Monzani, T., and Morselli, M. E., and Moskalenko, A., and Negro, I. V., and Nuss, M., and Orienti, E., and Orlando, M., and Ormes, E., and Paneque, J. F., and Perkins, D., and Pesce-Rollins, J. S., and Piron, M., and Pivato, F., and Porter, G., and Rainò, T. A., and Rando, S., and Razzano, R., and Reimer, M., and Reimer, A., and Reposeur, O., and Schmid, T., and Schulz, J., and Sgrò, A., and Simone, C., and Siskind, D., and Spada, E. J., and Spandre, F., and Spinelli, G., and Thayer, P., and Tibaldo, J. B., and Torres, L., D. F., Tosti, G., And, Troja, and Uchiyama, E., and Vianello, Y., and Vink, G., and Wood, J., and Yassine, K. S.
Publikováno v:
Astrophys.J.
Astrophys.J., 2016, 819 (2), pp.98. ⟨10.3847/0004-637X/819/2/98⟩
The astrophysical journal / 1 819(2), 98 (2016). doi:10.3847/0004-637X/819/2/98
Astrophysical Journal, 819(2):98. IOP Publishing Ltd.
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astrophys.J., 2016, 819 (2), pp.98. ⟨10.3847/0004-637X/819/2/98⟩
The astrophysical journal / 1 819(2), 98 (2016). doi:10.3847/0004-637X/819/2/98
Astrophysical Journal, 819(2):98. IOP Publishing Ltd.
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier \textit{Fermi} Large Area Telescope results reported the detection of $\gamma$-ray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8386add10fba9bcb3426537fecace3e
http://hdl.handle.net/11577/3209609
http://hdl.handle.net/11577/3209609